Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Aveek Sarkar"'
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 1, p 16 (2023)
Stream interaction regions (SIRs) are often thought to be responsible for the generation of suprathermal population in the interplanetary medium. Even though the source is the same, wide variations in the spectral indices of suprathermal populations
Externí odkaz:
https://doaj.org/article/5bfbb6463af548b3b0e46951091ff460
Autor:
Biswajit Mondal, Santosh V. Vadawale, Giulio Del Zanna, N. P. S. Mithun, Aveek Sarkar, Helen E. Mason, P. Janardhan, Anil Bhardwaj
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 2, p 146 (2023)
The first ionization potential (FIP) bias, whereby elemental abundances for low-FIP elements in different coronal structures vary from their photospheric values and may also vary with time, has been widely studied. In order to study the temporal vari
Externí odkaz:
https://doaj.org/article/53497b9349ca4658b65ea520b62b1790
Autor:
Biswajit Mondal, James A Klimchuk, Santosh V. Vadawale, Aveek Sarkar, Giulio Del Zanna, P. S. Athiray, N. P. S. Mithun, Helen E. Mason, Anil Bhardwaj
Publikováno v:
The Astrophysical Journal, Vol 945, Iss 1, p 37 (2023)
Small-scale impulsive events, known as nanoflares, are thought to be one of the prime candidates that can keep the solar corona hot at its multimillion-Kelvin temperature. Individual nanoflares are difficult to detect with the current generation of i
Externí odkaz:
https://doaj.org/article/527132ea13e0407084dc55cf2827cf6d
Recent high-resolution imaging and spectroscopic observations have generated renewed interest in spicules' role in explaining the hot corona. Some studies suggest that some spicules, often classified as type II, may provide significant mass and energ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af7080b4e857eae2ca0db435c112d5a7
http://arxiv.org/abs/2208.05240
http://arxiv.org/abs/2208.05240
Autor:
Biswajit Mondal, Shyama Narendranath, N. P. S. Mithun, Urmila Mitra-Kraev, Giulio Del Zanna, P. Janardhan, Helen E. Mason, Aveek Sarkar, Santosh V. Vadawale
The Solar X-ray Spectrometer (XSM) payload onboard Chandrayaan-2 provides disk-integrated solar spectra in the 1-15 keV energy range with an energy resolution of 180 eV (at 5.9 keV) and a cadence of 1~second. During the period from September 2019 to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c59ebd12a24349ba1ba41fa4a9061b0f
http://arxiv.org/abs/2107.07825
http://arxiv.org/abs/2107.07825
Interplanetary Coronal Mass Ejection (ICME) shocks are known to accelerate particles and contribute significantly to Solar Energetic Particle (SEP) events. We have performed Magnetohydrodynamic-Particle in Cell (MHD-PIC) simulations of ICME shocks to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6af8c4d36d313baa0d6735ddd3a7600d
http://hdl.handle.net/2318/1827280
http://hdl.handle.net/2318/1827280
Autor:
Tejas N. Sarvaiya, Santosh V. Vadawale, Partha Konar, Prashant Jangid, N. P. S. Mithun, Mahesh P Shanmugam, Aaditya Sarda, Girish D. Padia, Aveek Sarkar, Arpit R. Patel, D. K. Chakrabarty, Manan S. Shah, Prashant Kumar, Anil Bhardwaj
Solar X-ray Monitor (XSM) instrument of India's Chandrayaan-2 lunar mission carries out broadband spectroscopy of the Sun in soft X-rays. XSM, with its unique features such as low background, high time cadence, and high spectral resolution, provides
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::622164387ec53e65ded609a1bad02d01
Autor:
S. K. Goyal, Aaditya Sarda, Arpit R. Patel, M. Shanmugam, P. R. Adhyaru, Hiteshkumar L. Adalja, Tinkal Ladiya, D. K. Chakrabarty, K. P. Subramanian, Neeraj Kumar Tiwari, M. Chauhan, S. Banerjee, R.R. Bhavsar, M.B. Dadhania, Aveek Sarkar, Manan S. Shah, A. K. Hait, Santosh V. Vadawale, B. Bapat, P. Janardhan, Prashant Kumar
Publikováno v:
Planetary and Space Science. 163:42-55
The Aditya Solarwind Particle EXperiment (ASPEX) is one of the seven scientific payloads onboard the Aditya-L1 mission (the forthcoming Indian solar mission), to be placed in a halo orbit around the L1 Lagrangian point of the Sun-Earth system, at a d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fcbb0a87ecfbf99b4f927a1e7804eac0
https://doi.org/10.1016/j.pss.2018.04.008
https://doi.org/10.1016/j.pss.2018.04.008
Autor:
Tinkal Ladiya, Sushil Kumar, Arpit R. Patel, Shiv Kumar Goyal, Mahesh P Shanmugam, Anil Bhardwaj, P. Janardhan, Hitesh Kumar L. Adalja, N. P. S. Mithun, Neeraj Kumar Tiwari, Biswajit Mondal, Aveek Sarkar, Nishant Singh, Santosh V. Vadawale, Bhuwan Joshi
Publikováno v:
The Astrophysical Journal Letters. 912:L13
Solar flares, with energies ranging over several orders of magnitude, result from impulsive release of energy due to magnetic reconnection in the corona. Barring a handful, almost all microflares observed in X-rays are associated with the solar activ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c67e6364802a1376398592a719984e8f
https://doi.org/10.3847/2041-8213/abf0b0
https://doi.org/10.3847/2041-8213/abf0b0
Autor:
Santosh V. Vadawale, Bhuwan Joshi, Sushil Kumar, Tinkal Ladiya, Neeraj Kumar Tiwari, Shiv Kumar Goyal, Aveek Sarkar, P. Janardhan, Anil Bhardwaj, Mahesh P Shanmugam, Hitesh Kumar L. Adalja, Biswajit Mondal, Nishant Singh, N. P. S. Mithun, Arpit R. Patel
Publikováno v:
The Astrophysical Journal Letters. 912:L12
Elements with low First Ionization Potential (FIP) are known to be three to four times more abundant in active region loops of the solar corona than in the photosphere. There have been observations suggesting that this observed "FIP bias" may be diff
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::90b20ba3675c2b6f933deb4c6449ca6f
https://doi.org/10.3847/2041-8213/abf35d
https://doi.org/10.3847/2041-8213/abf35d