E-LIB Suche - Ergebnisse für: Boro Saikia, Sudeshna

1

Machine learning as a tool to determine exoplanet propertie:

Hajnik, Thomas ; Schanz, Andreas ; Boro Saikia, Sudeshna
doi:10.5281/zenodo.7739796. , 2023

Link: https://zenodo.org/recor..

2

NIRwave: A wave-turbulence-driven solar wind model constrai..:

Schleich, Simon ; Boro Saikia, Sudeshna ; Ziegler, Udo..
doi:10.5281/zenodo.7761619. , 2023

Link: https://zenodo.org/recor..

3

A change in the relationship between chromospheric activity..:

Brown, Emma, L ; Jeffers, Sandra, V ; Marsden, Stephen, C...
info:eu-repo/semantics/altIdentifier/doi/10.5281/zenodo.7344161. , 2022

Link: https://hal.science/hal-..

4

Modeling Coronal Mass Ejection Induced Dimmings on Epsilon ..:

Jin, Meng ; Loyd, Parke R. O ; Boro Saikia, Sudeshna...
doi:10.5281/zenodo.7379490. , 2022

Link: https://zenodo.org/recor..

5

A change in the relationship between chromospheric activity..:

Brown, Emma, L ; Jeffers, Sandra, V ; Marsden, Stephen, C...
info:eu-repo/semantics/altIdentifier/doi/10.5281/zenodo.7344161. , 2022

Link: https://hal.science/hal-..

6

A change in the relationship between chromospheric activity..:

Brown, Emma, L ; Jeffers, Sandra, V ; Marsden, Stephen, C...
info:eu-repo/semantics/altIdentifier/doi/10.5281/zenodo.7344161. , 2022

Link: https://hal.science/hal-..

7

A change in the relationship between chromospheric activity..:

Brown, Emma, L ; Jeffers, Sandra, V ; Marsden, Stephen, C...
info:eu-repo/semantics/altIdentifier/doi/10.5281/zenodo.7344161. , 2022

Link: https://hal.science/hal-..

8

A change in the relationship between chromospheric activity..:

Brown, Emma, L ; Jeffers, Sandra, V ; Marsden, Stephen, C...
info:eu-repo/semantics/altIdentifier/doi/10.5281/zenodo.7344161. , 2022

Link: https://hal.science/hal-..

9

A change in the relationship between chromospheric activity..:

Brown, Emma, L ; Jeffers, Sandra, V ; Marsden, Stephen, C...
info:eu-repo/semantics/altIdentifier/doi/10.5281/zenodo.7344161. , 2022

Link: https://hal.science/hal-..

10

Do non-dipolar magnetic fields contribute to spin-down torq..:

See, Victor ; Matt, Sean P ; Finley, Adam J...
https://research.usq.edu.au/download/4f3e3e7c85611d6e605a154a12030e37a20ddd077e530a01f39fa4c929d4930b/924035/See2_pub_2019.pdf. , 2019

Link: https://research.usq.edu..

11

Estimating magnetic filling factors from Zeeman–Doppler mag..:

See, Victor ; Matt, Sean P ; Folsom, Colin P...
https://research.usq.edu.au/download/d20a4d9b698aa8584c262e9bf9e60309a573fbf2ee4e757edb6121747e2ce317/595215/See2019.pdf. , 2019

Link: https://research.usq.edu..

12

Magnetic and activity cycles of cool stars:

Boro Saikia, Sudeshna
http://hdl.handle.net/11858/00-1735-0000-0023-3F34-4. , 2017

Link: http://hdl.handle.net/11..

13

The magnetic field geometry of cool stars:

See, Victor ; Jardine, Moira ; Vidotto, Aline...
https://zenodo.org/communities/cs19. , 2016

Link: https://zenodo.org/recor..

14

Airy worlds or barren rocks? On the survivability of second..:

Van Looveren, Gwenaël ; Güdel, Manuel ; Saikia, Sudeshna Boro.
http://arxiv.org/abs/2401.16490. , 2024

Link: http://arxiv.org/abs/240..

15

NIRwave: A wave-turbulence-driven solar wind model constrai..:

Schleich, Simon ; Saikia, Sudeshna Boro ; Ziegler, Udo..
http://arxiv.org/abs/2302.06493. , 2023

Link: http://arxiv.org/abs/230..