Skip to main content
This website is in trial operation, support us!
We gratefully acknowledge support from all contributors.
Contribute Donate

Astrophysics > Solar and Stellar Astrophysics

arXiv:2508.00661 (astro-ph)
[Submitted on 1 Aug 2025 ]

Title: The CUbesat Solar Polarimeter (CUSP): mission overview II

Title: CUbesat太阳偏振计（CUSP）：任务概述 II

Authors:Sergio Fabiani, Ettore Del Monte, Andrea Alimenti, Riccardo Campana, Mauro Centrone, Enrico Costa, Nicolas De Angelis, Giovanni De Cesare, Sergio Di Cosimo, Giuseppe Di Persio, Abhay Kumar, Alessandro Lacerenza, Pasqualino Loffredo, Giovanni Lombardi, Lorenzo Marra, Gabriele Minervini, Fabio Muleri, Paolo Romano, Alda Rubini, Emanuele Scalise, Enrico Silva, Paolo Soffitta, Davide Albanesi, Ilaria Baffo, Daniele Brienza, Valerio Campamaggiore, Giovanni Cucinella, Andrea Curatolo, Giulia de Iulis, Andrea Del Re, Vito Di Bari, Simone Di Filippo, Immacolata Donnarumma, Pierluigi Fanelli, Nicolas Gagliardi, Paolo Leonetti, Matteo Mergè, Dario Modenini, Andrea Negri, Daniele Pecorella, Massimo Perelli, Alice Ponti, Francesca Sbop, Paolo Tortora, Alessandro Turchi, Valerio Vagelli, Emanuele Zaccagnino, Alessandro Zambardi, Costantino Zazza
Abstract: The CUbesat Solar Polarimeter (CUSP) project is an Earth-orbiting CubeSat mission designed to measure the linear polarization of solar flares in the hard X-ray band using a Compton scattering polarimeter. CUSP will enable the study of magnetic reconnection and particle acceleration within the Sun's flaring magnetic structures. This project is being developed within the framework of the Italian Space Agency's Alcor Program, which aims to foster new CubeSat missions. CUSP entered its Phase B in December 2024, a phase scheduled to last 12 months. This paper reports on the current status of the CUSP mission design, mission analysis, and payload scientific performance.
Comments: Proceeding of the conference "SPIE Optics + Photonics 2025", 3 - 7 August 2025 San Diego, California, US
Subjects: Solar and Stellar Astrophysics (astro-ph.SR) ; Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:2508.00661 [astro-ph.SR]
  (or arXiv:2508.00661v1 [astro-ph.SR] for this version)
  https://doi.org/10.48550/arXiv.2508.00661

Submission history

From: Sergio Fabiani [view email]
[v1] Fri, 1 Aug 2025 14:27:51 UTC (1,760 KB)
Full-text links:

Access Paper:

license icon view license
Current browse context:
astro-ph.SR
< prev   |   next >
new | recent | 2025-08
Change to browse by:
astro-ph
astro-ph.IM

References & Citations

export BibTeX citation

Bookmark

BibSonomy logo Reddit logo

Bibliographic and Citation Tools

Bibliographic Explorer (What is the Explorer?)
Connected Papers (What is Connected Papers?)
Litmaps (What is Litmaps?)
scite Smart Citations (What are Smart Citations?)

Code, Data and Media Associated with this Article

alphaXiv (What is alphaXiv?)
CatalyzeX Code Finder for Papers (What is CatalyzeX?)
DagsHub (What is DagsHub?)
Gotit.pub (What is GotitPub?)
Hugging Face (What is Huggingface?)
Papers with Code (What is Papers with Code?)
ScienceCast (What is ScienceCast?)

Demos

Replicate (What is Replicate?)
Hugging Face Spaces (What is Spaces?)
TXYZ.AI (What is TXYZ.AI?)

Recommenders and Search Tools

Influence Flower (What are Influence Flowers?)
CORE Recommender (What is CORE?)
IArxiv Recommender (What is IArxiv?)

arXivLabs: experimental projects with community collaborators

arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.

Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.

Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.

Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)