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Journal articles on the topic 'Maitri'

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Author: Grafiati

Published: 6 September 2023

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1

SINGH, O. P., U. P. SINGH, and R. P. LAL. "Recent trends and variations in surface meteorological parameters over Indian Antarctic station Maitri." MAUSAM 62, no. 4 (December 16, 2021): 547–56. http://dx.doi.org/10.54302/mausam.v62i4.341.

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Utilizing surface meteorological data of temperature, pressure and wind of recent two decades, 1991-2010 over Indian Antarctic research station Maitri the trends and variabilities in surface meteorological parameters have been discussed. The trend in mean air temperature at Maitri has been -0.4/decade during past two decades showing no impact of global warming on Maitri surface temperature. There is no trend in surface pressure at Maitri during last two decades. Mean surface wind speed has shown slight increasing trend during the decade 1991-2000 whereas it has shown slight decreasing trend during the decade 2001-2010. However, there are large interannual variations in surface parameters and the linear trends seem to be the result of such variations. During Jan-March of two contrasting monsoon years 2009 and 2010 interesting anomalies in surface pressure at Maitri have been observed. Surface pressure was anomalously lower at Matri in Jan-March of drought year 2009 whereas positive pressure anomalies prevailed during the same period of excess monsoon year 2010. Negative temperature anomalies during January-March over Maitri preceded drought monsoon 2009 and positive anomalies prevailed during the same period before good monsoon 2010.

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2

TYAGI, AJIT, U. P. SINGH, and M. MOHAPATRA. "Weather & weather systems at Schirmacher Oasis (Maitri) during recent two decades - A review." MAUSAM 62, no. 4 (December 16, 2021): 513–34. http://dx.doi.org/10.54302/mausam.v62i4.337.

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Indian Antarctic station Maitri experiences varying external influences from interior of east Antarctica as well as moving depressions and cyclones along the coast. The relative position of circumpolar trough and strengthening of high pressure centre near pole influences variation of atmospheric pressure at Maitri. The diurnal, daily and seasonal variation of temperature mainly depend upon moving pressure systems, katabatic winds, change of solar insulation with change of seasons, reflectivity from clouds and snow surface. The katabatic winds prevail over Maitri which is highly directional from South- East sector due to increase of slope towards south. The blizzards are main weather at Maitri, fog and white out are occasional phenomena. The precipitation is mostly in form of snowfall but rain is very rare at Maitri. Heavy or moderate snowfall indicative of active front leading edge of warm air masses being transported southwards. Strong temperature variant near Schirmacher oasis give precipitation in form of snow. Fog occurred due to slow movement of relatively warm air from lower latitude over the colder surface. Winter season witnessed more snowfall accumulation at Maitri than other season. During summer rise of temperature accompanied with absorption of latent heat by ice pellets in low level of atmosphere results precipitation in form of water droplets. Highest number of blizzards occurs during winter season whereas lowest number of blizzards occurs during summer season. Normally due to cyclonic activities, warm air masses transported towards the Schirmacher oasis which causes rise of temperature at Maitri. Longer duration of the blizzards over the station depends upon strength of slow moving blocking anticyclone situated east of Maitri at lower latitude. Tremendous fluctuation of atmospheric electric field observed before onset is a pre-indication of commencement of blizzards.

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3

Chaubey, Jai Prakash, K. Krishna Moorthy, S. Suresh Babu, and Vijayakumar S. Nair. "The optical and physical properties of atmospheric aerosols over the Indian Antarctic stations during southern hemispheric summer of the International Polar Year 2007–2008." Annales Geophysicae 29, no. 1 (January 11, 2011): 109–21. http://dx.doi.org/10.5194/angeo-29-109-2011.

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Abstract. The properties of background aerosols and their dependence on meteorological, geographical and human influence are examined using measured spectral aerosol optical depth (AOD), total mass concentration (MT) and derived number size distribution (NSD) over two distinct coastal locations of Antarctica; Maitri (70° S, 12° E, 123 m m.s.l.) and Larsemann Hills (LH; 69° S, 77° E, 48 m m.s.l.) during southern hemispheric summer of 2007–2008 as a part of the 27th Indian Scientific Expedition to Antarctica (ISEA) during International Polar Year (IPY). Our investigations showed comparable values for the mean columnar AOD at 500 nm over Maitri (0.034±0.005) and LH (0.032±0.006) indicating good spatial homogeneity in the columnar aerosol properties over the coastal Antarctica. Estimation of Angstrom exponent α showed accumulation mode dominance at Maitri (α~1.2±0.3) and coarse mode dominance at LH (0.7±0.2). On the other hand, mass concentration (MT) of ambient aerosols showed relatively high values (≈8.25±2.87 μg m−3) at Maitri in comparison to LH (6.03±1.33 μg m−3).

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4

Keating, Christine. "Towards the Well-being of All: B.R. Ambedkar, Maitri, and Non-Fraternalist Democratic Solidarity." Comparative Political Theory 1, no. 2 (December 30, 2021): 273–78. http://dx.doi.org/10.1163/26669773-bja10022.

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Abstract In Buddhist thought, the cultivation of maitri, often defined as loving-kindness, involves the development of a commitment to the well-being of all. Drawing on the analysis of B.R. Ambedkar’s thought that Luis Cabrera presents in The Humble Cosmopolitan, this article explores Ambedkar’s endorsement of the Buddhist concept of maitri over fraternity as an alternative conceptualization of democratic solidarity.

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5

Bhawre, P., A. K. Gwal, A. A. Mansoori, and P. A. Khan. "Study of GPS derived Total Electron Content and Scintillation Index variations over Indian Arctic and Antarctic stations." Journal of Scientific Research 5, no. 2 (April 22, 2013): 255–64. http://dx.doi.org/10.3329/jsr.v5i2.12724.

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In the present study we have investigated the monthly and seasonal variability of total electron content (TEC) and amplitude scintillation index (S4) over two Indian polar stations Maitri (Antarctic) and Ny-Alesund (Arctic), during the low solar activity period 2008. We have used the Novatels dual frequency GPS receiver GSV4004A to accomplish this study. From our analysis we observed that TEC achieves its highest values during the months of November and December while during the month of May and June the lowest values of TEC were recorded at Maitri station. Similarly during summer season the highest values of TEC are recorded while in winter season lowest values of TEC are observed. The scintillations that occurred during the year 2008 at Maitri as well as at Ny-Alesund were generally found to be of weak type (S4?0.1), although few cases of moderate (S4?0.3) and strong (S4?0.5) scintillation were also observed. The occurrence characteristics of scintillations showed that maximum scintillations at Maitri occur during the month of July and August while least scintillations occur during the month of January and February. This type of ionospheric variability can be explained on the basis of solar irradiance at Polar Regions.Keywords: Total electron content; Scintillation index; Polar ionosphere.© 2013 JSR Publications. ISSN: 2070-0237 (Print); 2070-0245 (Online). All rights reserved.doi: http://dx.doi.org/10.3329/jsr.v5i2.12724 J. Sci. Res. 5 (2), 255-264 (2013)

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6

TIWARI, V. S. "Measurement of Ozone at Maitri, Antarctica." MAUSAM 50, no. 2 (December 17, 2021): 203–10. http://dx.doi.org/10.54302/mausam.v50i2.1848.

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Regular ozone profile measurement over Antarctica has been made by India Meteorological Department since 1987 at Dakshin Gangotri and later at Maitri (70.7°S, 11.7°E) since 1990 with the help of Indian electro-chemical ozone sonde. Surface ozone measurement was also started at Dakshin Gangotri since 1989 and later at Maitri. Ozone sonde data at Dakshin Gangotri and Maitri have been analysed and ozone hole structure has been studied in detail. The drastic decrease in ozone amount is clearly seen between 100 hPa to 30 hPa layer reaching near zero value. Incidently this is the layer where highest ozone concentration occurs during other months except September-October. The ozone hole has been quite severe during 1994-95 with increase in area and depth. During 1996 the Antarctic ozone hole was also similar to previous years. An interesting feature of the 1995 event was the persistence of ozone hole through November & December. Stratospheric temperature changes during 1995 also support that the cold core vortex during 1995 was very cold and persisted up to November.

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7

KULANDAIVELU, E., M. J. NARASIMHALU, and M. V. GUHAN. "FOG AT MAITRI, EAST ANTARCTICA." MAUSAM 58, no. 4 (November 26, 2021): 569–71. http://dx.doi.org/10.54302/mausam.v58i4.1451.

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8

Jerry Setiawan, Ikram, Indrayani Indrayani, Muammar Khaddafi, Yanita Yanita, and Henny Irawati. "EFFECT OF WORK SPIRIT AND WORK MOTIVATION ONEMPLOYEE ENGAGEMENT IN THE TANJUNGPINANG BUMI RESTAURANT (VEGETARIAN)." MORFAI JOURNAL 2, no. 1 (March 29, 2022): 39–42. http://dx.doi.org/10.54443/morfai.v2i1.197.

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This research aims to know the influence of the variable work spirit and motivation towards Employee Engagement at the restaurant Bumi Maitri (Vegetarian) Tanjungpinang. The study used quantitative associative methods with a population of 42 respondents at the Maitri Earth Restaurant (Vegetarian) Tanjungpinang. The results of the study were Y = 50,503 + 0, 461X1 + 0, 552X2 + E and the value of coefficient of determination (R2) amounted to 0.245 or 24.5%. The results of a variable T-test of the work spirit towards employee engagement at the obtained value probability Signifkasi of 0.002 < 0.05 and the value of Thitung 3.309 > this 1.68385.. Work motivation variables against employee engagement at the obtained probability signified value of 0,009 < 0.05 and Thitung value 2.756 > this 1.68385. The results of this study showed that the working motivation variable partially affected the employee engagement in the restaurant Bumi Maitri (Vegetarian) Tanjungpinang. The test results of the working spirit and the motivation of work affect employee engagement with the value of Fcalculate 7.641 > Ftabel3, 24th. The value of Adjusted R Square is 0.245 or 24.5%. The remaining 75.5% is influenced by other variables not examined in this study.

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9

BHOWMIK, S. K. ROY, ANUPAM KUMAR, and ANANDA K.DAS. "Real-time mesoscale modeling for short range prediction of weather over Maitri region in Antarctica." MAUSAM 62, no. 4 (December 16, 2021): 535–46. http://dx.doi.org/10.54302/mausam.v62i4.339.

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The main objective of this paper is to implement Polar WRF model for the Maitri (Lat. 70° 45 S, Long. 11° 44 E) region at the horizontal resolution of 15 km using initial and boundary conditions of the Global Forecast System T-382 operational at the India Meteorological Department (IMD). The study evaluates the performance of the model using the conventional approach of case studies. The results of the case studies illustrated in this paper reveal that the model is capable of capturing synoptic and meso-scale weather systems. Forecast fields are consistent with the corresponding analysis fields. Synoptic charts of mean sea level pressure prepared by the Weather Service of South Africa at Pretoria are used for the model validation. The model derived meteograms of mean sea level pressure are compared against the corresponding observations. The study demonstrates the usefulness of the forecast products for short range forecasting of weather over the Maitri region. The forecast outputs are made available in the real-time mode in the national web site of IMD www.imd.gov.in. The study is expected to benefit weather forecasters at Maitri.

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10

OKADA, Mamiko. "Blood-giving (1) Maitri (a) bala." JOURNAL OF INDIAN AND BUDDHIST STUDIES (INDOGAKU BUKKYOGAKU KENKYU) 43, no. 1 (1994): 318–14. http://dx.doi.org/10.4259/ibk.43.318.

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11

Ganguly, Nandita D. "Comparative Study of the Influence of Air Pollution on UVI at Maitri in Antarctica and New Delhi in India." ISRN Meteorology 2012 (November 16, 2012): 1–5. http://dx.doi.org/10.5402/2012/315859.

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The influence of air pollution on the erythemal ultraviolet irradiance (UVI) reaching the earth's surface has been investigated at the Indian Antarctic station Maitri and compared with that at New Delhi, the capital of India, over a period of three years from 2005 to 2007. Total ozone column (TOC), surface ozone, NO2 column, middle tropospheric SO2 column, and BrO column are observed to exhibit a deceasing trend at Maitri, having a clean and pristine environment, while UVI and aerosol optical depth at 500 nm exhibit an increasing trend. This negative correlation suggests that O3, NO2, SO2, and BrO act as filters against erythemal ultraviolet irradiance reaching the earth's surface, while the aerosols, which are present in the atmosphere of Maitri, may not be either very effective in filtering out the UVI reaching the earth's surface or may not be large enough to produce measurable effects on UVI. TOC and BrO column are observed to exhibit a deceasing trend at New Delhi, having comparatively higher levels of pollution, while UVI, NO2 column, middle tropospheric SO2 column, surface ozone, and aerosol optical depth at 500 nm exhibit an increasing trend. This suggests that TOC and BrO act as filters against UVI, while NO2, surface ozone, SO2, and aerosols in the atmosphere of New Delhi may not be large enough to produce measurable effects on UVI.

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12

KULANDAIVELU, E., and S. K. PESHIN. "Measurement of total ozone, D-UV radiation, sulphur dioxide and nitrogen dioxide with Brewer spectrophotometer at Maitri, Antarctica during 2000." MAUSAM 54, no. 2 (April 1, 2003): 505–10. http://dx.doi.org/10.54302/mausam.v54i2.1537.

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The latest state-of-art equipment called Brewer Ozone Spectrophotometer has been installed at Maitri, the permanent Indian Scientific Research Station, Antarctica in July 1999 to monitor total ozone, damaging part of ultra-violet radiation (D-UV), sulphur dioxide (SO2) and nitrogen dioxide (NO2). The depletion of ozone and its fluctuation were monitored day by day during Antarctic spring season (August-October). The data collected during the year 2000 are analysed in this paper. The values of total ozone and D-UV are compared in each month. The sudden increase or decrease of D-UV confirms further depletion or recovery of ozone in the successive days during the spring season. The measurements confirm the existence of 'Ozone Hole' over Antarctica 2000. The measurements of SO2 and NO2 at Maitri show very low values.

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13

Meena, Rajanti. "Maitri Pushpa ke Sahitye Mae Nari Chetna." National Journal of Environment and Scientific Research 2, no. 8 (August 22, 2021): 28. http://dx.doi.org/10.53571/njesr.2021.2.8.28-35.

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14

Naithani, Jaya, H. N. Dutta, P. K. Pasricha, B. M. Reddy, and K. M. Aggarwal. "Evaluation of turbulent fluxes over Maitri, Antarctica." Boundary-Layer Meteorology 74, no. 1-2 (April 1995): 195–208. http://dx.doi.org/10.1007/bf00715717.

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15

Deshpande, C. G., and A. K. Kamra. "Physical properties of aerosols at Maitri, Antarctica." Journal of Earth System Science 113, no. 1 (March 2004): 1–25. http://dx.doi.org/10.1007/bf02701995.

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16

BHASKAR, VVIZAYA. "AEROSOL OPTICAL THICKNESS OVER INDIAN ANTARCTICA STATION MAITRI." MAUSAM 65, no. 2 (April 1, 2014): 261–63. http://dx.doi.org/10.54302/mausam.v65i2.1008.

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17

Siingh, Devendraa, R. P. Singh, V. Gopalakrishnan, C. Selvaraj, and C. Panneerselvam. "Fair-weather atmospheric electricity study at Maitri (Antarctica)." Earth, Planets and Space 65, no. 12 (December 2013): 1541–53. http://dx.doi.org/10.5047/eps.2013.09.011.

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18

Nair, Sushma R., and D. S. Ramteke. "Environmental status at the Indian Antarctic station — Maitri." International Journal of Environmental Studies 56, no. 6 (September 1999): 869–87. http://dx.doi.org/10.1080/00207239908711245.

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19

Pant, Vimlesh, Devendraa Siingh, and A. K. Kamra. "Size distribution of atmospheric aerosols at Maitri, Antarctica." Atmospheric Environment 45, no. 29 (September 2011): 5138–49. http://dx.doi.org/10.1016/j.atmosenv.2011.06.028.

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20

Ganguly, N. D. "High surface ozone episodes at Maitri in Antarctica." Indian Journal of Physics 87, no. 10 (May 28, 2013): 947–51. http://dx.doi.org/10.1007/s12648-013-0325-1.

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21

PESIHN, S. K., P. RAJESH RAO, and S. K. SRIVASTAV. "Antarctic ozone depletion measured by balloonsondes at Maitri - 1992." MAUSAM 48, no. 3 (December 15, 2021): 443–46. http://dx.doi.org/10.54302/mausam.v48i3.4311.

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ABSTRACT. Profiles from a series of balloon borne ozonesonde ascents are used to chart the development of the Antarctic depletion over Maitri in the austral spring of 1992. The vertical structure of the ozone layer is discussed, including the presence of stratification, which occurs at all stages of development. The main feature of 1992 ozonesonde flights is depletion of 97% in the months of September and October between 15-23 km, which is unique.

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22

SRIVASTAVA, ARUN, V. K. JAIN, and H. N. DUTTA. "Surface wind characterization at an Antarctic coastal station, Maitri." MAUSAM 55, no. 1 (January 19, 2022): 95–102. http://dx.doi.org/10.54302/mausam.v55i1.932.

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Surface winds in the atmosphere of Maitri (70.7º S, 11.7º E) a coastal Indian station have been analysed for the year 1992. Surface winds blow most frequently from the sector 165° ± 25°. Wind chill factor for the year 1992 shows that chilling is highest during the month of August and lowest during the month of January. Two cases of blizzards one during summer and another during winter have also been studied. Surface winds remained practically from the SE, SSE and SW sector during the blizzards.

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23

LAL, R. P. "SHORT PERIOD CLIMATOLOGY OF MAITRI, SCHIRMACHER OASIS, EAST ANTARCTICA." MAUSAM 57, no. 4 (November 26, 2021): 684–88. http://dx.doi.org/10.54302/mausam.v57i4.522.

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24

KULANDAIVELU, E., and SARBJIT SINGH. "A study of wind chill effect at Maitri, Antarctica." MAUSAM 46, no. 1 (January 1, 2022): 31–34. http://dx.doi.org/10.54302/mausam.v46i1.3157.

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The influence of meteorological parameters like wind and temperature determine the chillness upon the human body. The rate of heat removal from the human body by wind and low temperature was termed as Wind Chill by Siple and Passel (1945). Using the wind chill chart wind chill effects at Maitri, Antarctica during 1990 have been studied and compared with conventional value of monthly mean dry bulb and minimum temperatures. It has been observed that the wind chili temperature was about 15°-25°C lower than the dry bulb temperature when the wind speed exceeds 10 kt.

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25

Ali, Kaushar, D. K. Trivedi, and S. K. Sahu. "Surface ozone characterization at Larsemann Hills and Maitri, Antarctica." Science of The Total Environment 584-585 (April 2017): 1130–37. http://dx.doi.org/10.1016/j.scitotenv.2017.01.173.

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26

LAL, R. P., and SURESH RAM. "Climatology of blizzards over Schirmacher Oasis, east Antarctica." MAUSAM 60, no. 1 (November 27, 2021): 39–50. http://dx.doi.org/10.54302/mausam.v60i1.960.

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Weather in Antarctica is subject to frequent and sudden changes. Strong winds and blizzards dominate Antarctic weather. A combination of blowing snow, gale force wind and very low visibility is normally defined as blizzard. Meteorological data recorded at Indian Antarctic Station Maitri, in respect of blizzards recorded during the period 1990-2005 has been studied to find out climatological features of blizzards affecting Schirmacher Oasis. At Maitri the blizzard is mostly associated with extra-tropical storms and is normally preceded by precipitation. On average during the year about 21 blizzards affects the station for 45 days during the year. During the month of April to August 3 to 4 blizzards affects the station. Maximum number of blizzards occurs in the month of August with about 7 blizzard days. Average wind speed recorded during the blizzard is about 52 kt but it exceeded 100 kt on several occasions. The duration may vary from hours to days with average of 25 hours. Longest duration of 168 hours was recorded in June 1997. There are about 12 such occasions when blizzard lasted more than 72 hours. No correlation has been found between maximum wind speed and temperature rise during blizzard and the speed is also not correlated with pressure departure during the period.

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27

KULANDAIVELU, E., S. SRIDHARAN, and S. R. RAMANAN. "The effect of atmospheric blocking high and ridges on weather over Maitri, East Antarctica – A case study." MAUSAM 56, no. 2 (January 20, 2022): 375–84. http://dx.doi.org/10.54302/mausam.v56i2.940.

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The Indian Antarctic station, Maitri is often experiencing continuous blizzard over a week with strong surface winds and surface temperature anomalies due to atmospheric blocking during winter and spring seasons of Antarctica. One such case during the last week of August 2000 and another case in mid-July 1996 are studied. There is more blocking activity in winter and spring months. The influence of blocking high on weather parameters during the study period is also presented.

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28

Sari Sitompul, Silvia, and Wilbert Sentosa. "Pengaruh Pengembangan Karir, Kompetensi dan Pelatihan Terhadap Kinerja Karyawan Pada PT Maitri Mustika Abadi di Pekanbaru." Jurnal BANSI - Jurnal Bisnis Manajemen Akutansi 2, no. 1 (June 29, 2022): 10–20. http://dx.doi.org/10.58794/bns.v2i1.62.

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Tujuan penelitian ini adalah untuk mencari tahu besarnya pengaruh dan signifikan dari Pengembangan Karir, Kompetensi dan Pelatihan terhadap Kinerja pada PT Maitri Mustika Abadi Pekanbaru. Populasi penelitian ini adalah Karyawan Perusahaan dengan sampel penelitian 98 orang yang diambil dengan teknik pengambilan sampel jenuh, metode analisis yang digunakan metode Analisis Regresi Linear Berganda dengan SPSS v.20. Hasil penelitian ini menunjukkan bahwa pengembangan karir dan kompetensi mempengaruhi kinerja karyawan, sedangkan variabel pelatihan tidak mempengaruhi kinerja karyawan pada perusahaan ini.

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29

KASAI, Tadashi. "Nichiren's View of maitri-karuna: A Comparison with St. Bernard." JOURNAL OF INDIAN AND BUDDHIST STUDIES (INDOGAKU BUKKYOGAKU KENKYU) 39, no. 1 (1990): 214–20. http://dx.doi.org/10.4259/ibk.39.214.

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30

M, Rukmani. "Feminist portrayal in the poems of Salma and Malati Maitri." International Research Journal of Tamil 4, S-8 (August 9, 2022): 317–24. http://dx.doi.org/10.34256/irjt22s845.

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Tamil poets have created, named, categorized, summarized and preserved dialects based on dialects in order to preserve the language they speak. Before exploring the importance of numbers in language it is necessary to know the design of grammatical literature. It is possible that the Sanskrit poets called the text grammar of the words when they recorded the language, they created in the journals so that it would be known to the world, and the textual literature of the world empirical biographies based on his linguistic ability. By learning the language of counting and writing as the body and soul direct the human being, it is possible to know through the Tamil numerals that the numbers representing the measurements are also designed while the letters are being created. The purpose of the article is to give an overview of the measurements that have taken place in human life, with descriptions of messages, numbers, and nouns. The importance of numbers has been highlighted in explaining the alphabetical order of the letters and the alphabetical alphabets created for the Tamil language under the heading of letters and numbers, as well as the design of the vowels formed with the primary letters. The use of numbers in the classification of letters by alphabetical order is illustrated by the use of numbers to distinguish vowel letters into vowel, melody, and interjection types, and to point and quote characters. The words created for measurements such as size and mass are the primary letters of the words and the reasons for giving a special place to measurements in Tamil are explained. In order to give Tamil a lofty place in the world languages in the end, there are poems in which the Tamils use their numbers to indicate the year of publication, the year of an action, the time of action, and the number of soldiers involved in the war. The conclusion of the study is outlined.

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31

Basu, Ambar, and Parameswari Mukherjee. "India’s COVID vaccine gestures: from maitri to coloniality." Communication and Critical/Cultural Studies 19, no. 2 (April 3, 2022): 134–39. http://dx.doi.org/10.1080/14791420.2022.2064529.

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32

SHIZUKA, Haruki. "Expulsion of Maitri-pa from the Monastery and Atisa's Participation." Journal of Indian and Buddhist Studies (Indogaku Bukkyogaku Kenkyu) 63, no. 3 (2015): 1315–21. http://dx.doi.org/10.4259/ibk.63.3_1315.

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33

Siingh, Devendraa, Vimlesh Pant, and A. K. Kamra. "Temperature-dependence of the positive intermediate ion concentrations at Maitri, Antarctica." Journal of Atmospheric and Solar-Terrestrial Physics 104 (November 2013): 67–74. http://dx.doi.org/10.1016/j.jastp.2013.08.011.

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34

Naithani, Jaya, and H. N. Dutta. "Acoustic sounder measurements of the planetary boundary layer at Maitri, Antarctica." Boundary-Layer Meteorology 76, no. 1-2 (October 1995): 199–207. http://dx.doi.org/10.1007/bf00710897.

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35

Jeeva, K., C. Panneerselvam, K. U. Nair, C. Selvaraj, Ajay Dhar, B. M. Pathan, and S. Gurubaran. "Global electric circuit parameters and their variability observed over Maitri, Antarctica." Journal of the Geological Society of India 78, no. 3 (September 2011): 199–210. http://dx.doi.org/10.1007/s12594-011-0088-2.

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36

Patel, R. P., R. P. Singh, Ashok K Singh, A. K. Gwal, and D. Hamar. "Observation of very low frequency emissions at Indian Antarctic station, Maitri." Pramana 61, no. 4 (October 2003): 773–78. http://dx.doi.org/10.1007/bf02706127.

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37

BEHERA, JAYANTA K., A. K. SINHA, ANAND K. SINGH, RAHUL RAWAT, GEETA VICHARE, AJAY DHAR, B. M. PATHAN, K. U. NAIR, C. SELVARAJ, and P. ELANGO. "First results from imaging riometer installed at Indian Antarctic station Maitri." Journal of Earth System Science 123, no. 3 (April 2014): 593–602. http://dx.doi.org/10.1007/s12040-014-0412-5.

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38

Nakasone, Ronald Y. "Illness and Compassion: AIDS in an American Zen Community." Cambridge Quarterly of Healthcare Ethics 4, no. 4 (1995): 488–93. http://dx.doi.org/10.1017/s0963180100006319.

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In an interview just before his death, Issan Dorsey, an American Zen priest and abbot of the Hartford Street Zen Center, stated, “AIDS is not fatal. Life is fatal. If you have AIDS, you are alive.” Although infected with AIDS, Issan worked to establish the Maitri Hospice for those dying from complications related to AIDS in the San Francisco Castro District, the heart of the gay and lesbian community. His efforts reflect the statement–although the body may be diseased, one can continue to give abundantly and tirelessly, articulated by Vimalakirti in the Vimalakirtinirdesa Sutra (Sutra on the Teaching of Vimalakirti).

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HOSALIKAR, K. S., SUSHMA NAIR, and RAJIV KRISHNAMURTHY. "A short term characterisation of wind and temperature over Maitri, East Antarctica." MAUSAM 62, no. 4 (December 16, 2021): 567–76. http://dx.doi.org/10.54302/mausam.v62i4.350.

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Polar Science is gaining increased importance in Climate Change studies because of the profound influence Polar Climatology has on the Global Climate. Research shows that Antarctica seems to be warming around the edges and cooling at the center at the same time. East Antarctica is climatologically colder than west Antarctica because of its higher elevation. A short term characterization of wind and the temperature over Maitri is attempted in this paper. Maximum and Minimum temperatures showed a tendency to decrease with winter contributing the most to the change. The Wind Directions were predominantly South-South-Easterly in summer and autumn and South-Easterly in winter and spring, with katabatic winds showing the maximum frequency in autumn. The wind speeds were found to be most variable in winter. Greater contributions to the wind chill temperatures were found from the winds, with the tendency for change being more prominent in the transition seasons.

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Deshpande, C. G., and A. K. Kamra. "Diurnal variations of the atmospheric electric field and conductivity at Maitri, Antarctica." Journal of Geophysical Research: Atmospheres 106, no. D13 (July 1, 2001): 14207–18. http://dx.doi.org/10.1029/2000jd900675.

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Victor, N. Jeni, C. Panneerselvam, and C. P. Anil Kumar. "Variation of surface electric field during geomagnetic disturbed period at Maitri, Antarctica." Journal of Earth System Science 124, no. 8 (December 2015): 1721–33. http://dx.doi.org/10.1007/s12040-015-0638-x.

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Rajaram, Girija, T. Arun, Ajay Dhar, and A. G. Patil. "Rapid decrease in total magnetic field F at Antarctic stations - its relationship to core–mantle features." Antarctic Science 14, no. 1 (March 2002): 61–68. http://dx.doi.org/10.1017/s0954102002000585.

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The Indian Institute of Geomagnetism (IIG) in 1982, 1986, and 1996, operated a Proton Precession Magnetometer (PPM) at its Antarctic stations Dakshin Gangotri/Maitri (located at ∼70°S, ∼12°E). Comparison of the average quiet-time value of total intensity F for these years with values of F obtained at the same geographic location (interpolated from iso-intensity contours of F on World Magnetic Charts and IGRF Maps) for earlier years, suggested that over the last 75 years at this location, F has dropped from ∼49 000 nT in 1922, to ∼40 000 nT in 1996 i.e. ∼120 nT per year. Further inspection at nearby Antarctic stations reveals a drop of ∼108 nT yr−1 at Novolazarevskaya, ∼100 nT yr−1, at Georg Forster and ∼95 nT yr−1 at Syowa; Mawson situated still further away shows a drop of ∼72 nT yr−1, while Dumont d'Urville located very near the magnetic pole showed a drop of ∼50 nT yr−1 until 1994. A study of the observed F values over the past five decades at 23 observatories from the Antarctic and sub-Antarctic regions indicates that contours of yearly decrease in F follow a definite pattern, with maximum decrease lying in a belt encompassing Maitri. These observations are of importance in the light of modelling works at the Earth's Core–Mantle boundary pointing to two prominent regions of reverse magnetic flux (RMF) occurring beneath South America, South Africa and a large part of Antarctica, and which may merge sometime to cause reversal of the present geomagnetic field polarity. The importance of continuous monitoring of F at various locations in Antarctic and sub-Antarctic regions is brought out in this work. It is equally important to understand the cause behind this rapid decrease in F.

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SHARMA, A. K. "Applications of satellite imageries for prediction of severe weather events along Maitri, Antarctica." MAUSAM 62, no. 4 (December 16, 2021): 617–26. http://dx.doi.org/10.54302/mausam.v62i4.379.

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The present paper is an attempt to educate the weather forecaster at Indian Scientific research Station, Maitri, Antarctica in forecasting severe weather (blizzards) using satellite images of various satellites operating in the world. The Polar stationary satellite ‘Trianna’ has been discussed .The availability of the various types of images has also been spelt. The characteristics of satellite images has been described along with overlaying of Automatic Weather station (AWS) data explaining the occurrence of Katabatic winds which also causes blizzards. Blizzard conditions often develop on the northwest side of an intense storm system the difference between the lower pressure in the storm and the higher pressure to the west creates a tight pressure gradient, which in turn results in very strong winds or blizzards. The paper also discusses about the development that took place in Antarctic satellite meteorology since beginning.

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PESHIN, S. K. "Study of SO2 and NO2 behaviour during the ozone-hole event at Antarctica by Brewer Spectrophotometer." MAUSAM 62, no. 4 (December 16, 2021): 595–600. http://dx.doi.org/10.54302/mausam.v62i4.364.

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Vertical column density of sulphur dioxide has been measured at Maitri (70.7°S, 11.7°E), the Indian station in the Antarctica from September, 1999 to December, 2006 by a Brewer Spectrophotometer. Simultaneously, nitrogen dioxide, ozone and the maximum value of UV-B have also been measured, we found an increase in SO2 during spring. An increase in NO2 column was also found during this period but not identical with that of SO2. These variations in SO2 and NO2 are not in phase with the increase in UV-B flux at the ground due to the decrease of ozone column in the stratosphere. The variation of SO2 column is explained by the downward shift of penetration depth of UV-B radiation during the ozone-hole event.

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Suharno, Hariyanto, and Ngadat. "EKSISTENSI PENYULUH AGAMA BUDDHA DALAM MEMPERTAHANKAN KEYAKINAN UMAT BUDDHA DI VIHARA MAITRI RATNA DUSUN BEDUG DESA GEDONGREJO KECAMATAN GIRIWOYO KABUPATEN WONOGIRI JAWA TENGAH." NIVEDANA : Jurnal Komunikasi dan Bahasa 1, no. 1 (July 30, 2020): 69–84. http://dx.doi.org/10.53565/nivedana.v1i1.143.

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Penelitian ini bertujuan mendeskripsikan eksistensi penyuluh agama Buddha dalam mempertahankan keyakinan umat di Vihara Maitri Ratna Dusun Bedug, Desa Gedongrejo, Kecamatan Giriwoyo Kabupaten Wonogiri. Objek penelitian adalah penyuluh Agama Buddha Penelitian ini menggunakan metode penelitian kualitatif. Teknik pengumpulan data berasal dari wawancara dan observasi. Teknik analisis data yang digunakan adalah model interaktif yang mengklasifikasikan analisis data dalam tiga langkah yaitu reduksi, penyajian, dan penarikan simpulan. Hasil penelitian menunjukkan bahwa eksistensi penyuluh agama Buddha sangat dibutuhkan oleh masyarakat Buddha. Eksistensi penyuluh sebagai penggerak umat atau motivasi dalam mempertahankan keyakinan ajaran Buddha Dhamma. Seorang penyuluh memiliki tiga komponen penting dalam fungsi dan perannya sebagai seorang penyuluh, yaitu menggerakkan, mengarahkan, dan menopang tingkah laku manusia. Kompetensi penyuluh agama Buddha sangat membantu dalam pengetahuan dan wawasan umat Buddha.

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Singh, Jagdev. "Study of Calcium-K Network Evolution from Antarctica." International Astronomical Union Colloquium 141 (1993): 410–11. http://dx.doi.org/10.1017/s0252921100029535.

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AbstractTo study the evolution and decay of large convective cells known as supergranules, a solar telescope was set up at Maitri, Indian permanent station in Antarctica region during the local summer months (December 1989 through March 1990). A continuous sequence of calcium-K-line filtergrams for 106 hours with an interval of about 10 minute was obtained. The analysis of this data indicates that most probable life time of the calcium K network is about 20 hours. The life time depends upon the size of the cell and is larger for bigger cells. The data also show that cells (of given size) associated with remanent magnetic field regions live longer than those in the region free from magnetic field regions.

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Khatarkar, Prakash, Parvaiz A. Khan, Shivangi Bhardwaj, P. K. Purohit, Roshni Atulkar, and A. K. Gwal. "The statistical investigation of amplitude Scintillations at Indian high latitude Station Maitri, Antarctica." Journal of Physics: Conference Series 640 (September 28, 2015): 012071. http://dx.doi.org/10.1088/1742-6596/640/1/012071.

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Rajaram, Girija, A. N. Hanchinal, R. Kalra, K. Unnikrishnan, K. Jeeva, M. Sridharan, and A. Dhar. "Velocity of small-scale auroral ionospheric current systems over Indian Antarctic station Maitri." Journal of Earth System Science 111, no. 1 (March 2002): 51–62. http://dx.doi.org/10.1007/bf02702222.

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49

Akilan, A., S. Balaji, Y. Srinivas, and N. Yuvaraj. "Plate motion predictability using Hurst exponent applied to the Maitri-antarctica GPS network." Journal of the Geological Society of India 82, no. 6 (December 2013): 613–20. http://dx.doi.org/10.1007/s12594-013-0199-z.

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50

Babu, G. S. D. "First Indian astronomical observations in Antarctica." Highlights of Astronomy 9 (1992): 595. http://dx.doi.org/10.1017/s1539299600022644.

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An Indian expedition to Antarctica (to the coastal base Maitri) in the 1989/90 summer made observations of the Sun to study the evolution and decay of supergranules, an experiment which benefited greatly from uninterrupted sessions of a few days. The instrument comprised a heliostat, a 1.2 Å bandwidth blue filter, and a 10 cm aperture lens of about 3 metre focal length with recording on film. During January and February, one continuous period of more than 100 hours completely clear sky occurred, during which the transparency of the atmosphere was excellent. However, at times the seeing was a little poor. More than 2500 photographs were made at 10 minute intervals, as well as some at shorter intervals for studying the evolution of other solar features such as flares.

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