Publication data of Antia, H.M.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19851990199520002005201020152020202502505007501000125015001750
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19851990199520002005201020152020202502040608010001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1985199019952000200520102015202020250510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestA study of possible temporal and latitudinal variations in the properties of the solar tachoclineA study of possible temporal and latitudinal variations in the properties of the…Forbush decreases and turbulence levels at CME frontsHigh rigidity Forbush decreases: due to CMEs or shocks?AstroSat/LAXPC Detection of Millisecond Phenomena in 4U 1728-34Ring diagram analysis of near surface flows in the SunAstroSat and MAXI view of the black hole binary 4U 1630−472 during 2016 and 2018 outburstsAstroSat and MAXI view of the black hole binary 4U 1630−472 during 2016 …Estimate of solar radius from f-mode frequenciesBroad-band reflection spectroscopy of MAXI J1535–571 using AstroSat: estimation of black hole mass and spinBroad-band reflection spectroscopy of MAXI J1535–571 using AstroSat: estim…Asteroseismic determination of helium abundance in stellar envelopesTemporal variations of the rotation rate in the solar interiorAstroSat/LAXPC observation of Cygnus X-1 in the hard stateChanges in solar dynamics from 1995 to 2002Solar internal rotation rate and the latitudinal variation of the tachoclineDetermining solar abundances using helioseismologyThe sun's acoustic asphericity and magnetic fields in the solar convection zoneThe sun's acoustic asphericity and magnetic fields in the solar convection zo…The Discrepancy between solar abundances and helioseismologyAstroSat/LAXPC reveals the high-energy variability of GRS 1915+105 in the $chi$ classAstroSat/LAXPC reveals the high-energy variability of GRS 1915+105 in the $…Constraining solar abundances using helioseismologyHelioseismology and Solar Abundances19851990199520002005201020152020202502505007501000125015001750
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)A study of possible temporal and latitudinal variations in the properties of the solar tachoclineA study of possible temporal and latitudinal variations in the properties of the…Forbush decreases and turbulence levels at CME frontsHigh rigidity Forbush decreases: due to CMEs or shocks?AstroSat/LAXPC Detection of Millisecond Phenomena in 4U 1728-34Ring diagram analysis of near surface flows in the SunAstroSat and MAXI view of the black hole binary 4U 1630−472 during 2016 and 2018 outburstsAstroSat and MAXI view of the black hole binary 4U 1630−472 during 2016 …Estimate of solar radius from f-mode frequenciesBroad-band reflection spectroscopy of MAXI J1535–571 using AstroSat: estimation of black hole mass and spinBroad-band reflection spectroscopy of MAXI J1535–571 using AstroSat: estim…Asteroseismic determination of helium abundance in stellar envelopesTemporal variations of the rotation rate in the solar interiorAstroSat/LAXPC observation of Cygnus X-1 in the hard stateChanges in solar dynamics from 1995 to 2002Solar internal rotation rate and the latitudinal variation of the tachoclineDetermining solar abundances using helioseismologyThe sun's acoustic asphericity and magnetic fields in the solar convection zoneThe sun's acoustic asphericity and magnetic fields in the solar convection zo…The Discrepancy between solar abundances and helioseismologyAstroSat/LAXPC reveals the high-energy variability of GRS 1915+105 in the $chi$ classAstroSat/LAXPC reveals the high-energy variability of GRS 1915+105 in the $…Constraining solar abundances using helioseismologyHelioseismology and Solar Abundances1985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1985199019952000200520102015202020250255075100125