dc.contributor.author |
Tripathi, Durgesh |
|
dc.contributor.author |
Chakrabarty, D |
|
dc.contributor.author |
Nandi, A |
|
dc.contributor.author |
Prasad, B. R |
|
dc.contributor.author |
Ramaprakash, A. N |
|
dc.contributor.author |
Shaji, Nigar |
|
dc.contributor.author |
Sankarasubramanian, K |
|
dc.contributor.author |
Satheesh Thampi, R |
|
dc.contributor.author |
Yadav, V. K |
|
dc.date.accessioned |
2023-10-11T08:40:03Z |
|
dc.date.available |
2023-10-11T08:40:03Z |
|
dc.date.issued |
2023 |
|
dc.identifier.citation |
Proceedings of the International Astronomical Union, Vol. 18, No. S372, pp. 17-27 |
en_US |
dc.identifier.issn |
1743-9221 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/8270 |
|
dc.description |
Restricted Access |
en_US |
dc.description.abstract |
The Aditya-L1 is the first space-based solar observatory of the Indian Space Research Organization (ISRO). The spacecraft will carry seven payloads providing uninterrupted observations of the Sun from the first Lagrangian point. Aditya-L1 comprises four remote sensing instruments, viz. a coronagraph observing in visible and infrared, a full disk imager in Near Ultra-Violet (NUV), and two full-sun integrated spectrometers in soft X-ray and hard X-ray. In addition, there are three instruments for in-situ measurements, including a magnetometer, to study the magnetic field variations during energetic events. Aditya-L1 is truly a mission for multi-messenger solar astronomy from space that will provide comprehensive observations of the Sun across the electromagnetic spectrum and in-situ measurements in a broad range of energy, including magnetic field measurements at L1. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Cambridge University Press on behalf of International Astronomical Union |
en_US |
dc.relation.uri |
https://doi.org/10.1017/S1743921323001230 |
|
dc.rights |
© The Author(s), 2023 |
|
dc.subject |
Sun: abundances |
en_US |
dc.subject |
Sun: activity |
en_US |
dc.subject |
Sun: atmospheric motions |
en_US |
dc.subject |
Sun: atmosphere |
en_US |
dc.subject |
Sun: chromosphere |
en_US |
dc.subject |
Sun: corona |
en_US |
dc.subject |
Sun: coronal mass ejections (CMEs) |
en_US |
dc.subject |
Sun: faculae, plages |
en_US |
dc.subject |
Sun: filaments |
en_US |
dc.subject |
Sun: flares |
en_US |
dc.subject |
Sun: fundamental parameters |
en_US |
dc.subject |
Sun: general |
en_US |
dc.subject |
Sun: granulation |
en_US |
dc.subject |
Sun: infrared |
en_US |
dc.subject |
Sun: magnetic fields |
en_US |
dc.subject |
Sun: particle emission |
en_US |
dc.subject |
Sun: photosphere |
en_US |
dc.subject |
Sun: prominences |
en_US |
dc.subject |
Sun: solar-terrestrial relations |
en_US |
dc.subject |
Sun: solar wind |
en_US |
dc.subject |
Sun: sunspots |
en_US |
dc.subject |
Sun: UV radiation |
en_US |
dc.subject |
Sun: X-rays |
en_US |
dc.title |
The Aditya-L1 mission of ISRO |
en_US |
dc.type |
Article |
en_US |