An insight into India's Moon mission–Chandrayan-3: The first nation to land on the southernmost polar region of the Moon
With the mission's completion, India became only the fourth nation in history to successfully
perform a soft landing on the Moon and the first nation to land a spacecraft close to the lunar …
perform a soft landing on the Moon and the first nation to land a spacecraft close to the lunar …
Evolution of elemental abundances during b-class solar flares: soft x-ray spectral measurements with chandrayaan-2 XSM
B Mondal, A Sarkar, SV Vadawale… - The Astrophysical …, 2021 - iopscience.iop.org
Abstract The Solar X-ray Monitor (XSM) payload on board Chandrayaan-2 provides disk-
integrated solar spectra in the 1–15 keV energy range with an energy resolution of 180 eV …
integrated solar spectra in the 1–15 keV energy range with an energy resolution of 180 eV …
Identifying the energy release site in a solar microflare with a jet
AF Battaglia, W Wang, J Saqri, T Podladchikova… - Astronomy & …, 2023 - aanda.org
Context. One of the main science questions of the Solar Orbiter and Parker Solar Probe
missions deals with understanding how electrons in the lower solar corona are accelerated …
missions deals with understanding how electrons in the lower solar corona are accelerated …
Soft X-ray spectral diagnostics of multithermal plasma in solar flares with chandrayaan-2 XSM
Spectroscopic observations in X-ray wavelengths provide excellent diagnostics of the
temperature distribution in solar flare plasma. The Solar X-ray Monitor (XSM) on board the …
temperature distribution in solar flare plasma. The Solar X-ray Monitor (XSM) on board the …
Solar X-ray monitor on board the Chandrayaan-2 orbiter: in-flight performance and science prospects
Abstract The Solar X-ray Monitor (abbreviated as XSM) on board India's Chandrayaan-2
mission is designed to carry out broadband spectroscopy of the Sun from lunar orbit. It …
mission is designed to carry out broadband spectroscopy of the Sun from lunar orbit. It …
Observations of the quiet sun during the deepest solar minimum of the past century with Chandrayaan-2 XSM: sub-A-class microflares outside active regions
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 …
release of energy due to magnetic reconnection in the corona. Barring a handful, almost all …
Coronal elemental abundances during A-class solar flares observed by Chandrayaan-2 XSM
The abundances of low first ionization potential (FIP) elements are three to four times higher
in the closed loop active corona than in the photosphere, known as the FIP effect …
in the closed loop active corona than in the photosphere, known as the FIP effect …
Multiwavelength observations by XSM, hinode, and SDO of an active region. Chemical abundances and temperatures
G Del Zanna, B Mondal, YK Rao… - The Astrophysical …, 2022 - iopscience.iop.org
We have reviewed the first year of observations of the Solar X-ray Monitor (XSM) on board
Chandrayaan-2 and the available multiwavelength observations to complement the XSM …
Chandrayaan-2 and the available multiwavelength observations to complement the XSM …
Observations of the quiet sun during the deepest solar minimum of the past century with chandrayaan-2 xsm: elemental abundances in the quiescent corona
Elements with low first ionization potential (FIP) are known to be 3–4 times more abundant in
active region loops of the solar corona than in the photosphere. There have been …
active region loops of the solar corona than in the photosphere. There have been …
Multiwavelength Observations of a B-class Flare Using XSM, AIA, and XRT
YK Rao, B Mondal, G Del Zanna… - The Astrophysical …, 2023 - iopscience.iop.org
We present multiwavelength observations by Chandrayaan-2/Solar X-ray Monitor, Solar
Dynamics Observatory/Atmospheric Imaging Assembly, and Hinode/X-Ray Telescope (XRT) …
Dynamics Observatory/Atmospheric Imaging Assembly, and Hinode/X-Ray Telescope (XRT) …