Guardado en:
Detalles Bibliográficos
Autores principales: Kennea, Jamie A., Racusin, Judith L., Burns, Eric, Grefenstettte, Brian W., Hounsell, Rebekah A., Hui, C. Michelle, Kocevski, Daniel, Lazio, T. Joseph W., Lesage, Stephen, Pritchard, Tyler A., Tohuvavohu, Aaron, Tomsick, John A., Traore, David, Wilson-Hodge, Colleen A.
Formato: Preprint
Publicado: 2024
Materias:
Acceso en línea:https://arxiv.org/abs/2410.03980
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866914965454061568
author Kennea, Jamie A.
Racusin, Judith L.
Burns, Eric
Grefenstettte, Brian W.
Hounsell, Rebekah A.
Hui, C. Michelle
Kocevski, Daniel
Lazio, T. Joseph W.
Lesage, Stephen
Pritchard, Tyler A.
Tohuvavohu, Aaron
Tomsick, John A.
Traore, David
Wilson-Hodge, Colleen A.
author_facet Kennea, Jamie A.
Racusin, Judith L.
Burns, Eric
Grefenstettte, Brian W.
Hounsell, Rebekah A.
Hui, C. Michelle
Kocevski, Daniel
Lazio, T. Joseph W.
Lesage, Stephen
Pritchard, Tyler A.
Tohuvavohu, Aaron
Tomsick, John A.
Traore, David
Wilson-Hodge, Colleen A.
contents The Time-Domain And MultiMessenger (TDAMM) Communications Science Analysis Group (TDAMMCommSAG) was formulated to describe the unique technical challenges of communicating rapidly to and from NASA astrophysics missions studying the most variable, transient, and extreme objects in the Universe. This report describes the study of if and how the transition from current NASA-operated space and ground relays to commercial services will adequately serve these missions. Depending on the individual mission requirements and Concept of Operations (ConOps), TDAMM missions may utilize a rapid low-rate demand access service, a low-rate continuous contact service, low-latency downlink upon demand, or a higher-latency but regular relay service. The specific implementations can vary via space relay or direct to Earth, but requires flexibility and adaptability using modern software infrastructure. The study team reviewed the current state of NASA communications services and future commercial and NASA communications services under study and in development. We explored the communications capabilities driving from the behavior of the astrophysical objects themselves.
format Preprint
id arxiv_https___arxiv_org_abs_2410_03980
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Time-Domain And MultiMessenger Astrophysics Communications Science Analysis Group Report
Kennea, Jamie A.
Racusin, Judith L.
Burns, Eric
Grefenstettte, Brian W.
Hounsell, Rebekah A.
Hui, C. Michelle
Kocevski, Daniel
Lazio, T. Joseph W.
Lesage, Stephen
Pritchard, Tyler A.
Tohuvavohu, Aaron
Tomsick, John A.
Traore, David
Wilson-Hodge, Colleen A.
Instrumentation and Methods for Astrophysics
High Energy Astrophysical Phenomena
The Time-Domain And MultiMessenger (TDAMM) Communications Science Analysis Group (TDAMMCommSAG) was formulated to describe the unique technical challenges of communicating rapidly to and from NASA astrophysics missions studying the most variable, transient, and extreme objects in the Universe. This report describes the study of if and how the transition from current NASA-operated space and ground relays to commercial services will adequately serve these missions. Depending on the individual mission requirements and Concept of Operations (ConOps), TDAMM missions may utilize a rapid low-rate demand access service, a low-rate continuous contact service, low-latency downlink upon demand, or a higher-latency but regular relay service. The specific implementations can vary via space relay or direct to Earth, but requires flexibility and adaptability using modern software infrastructure. The study team reviewed the current state of NASA communications services and future commercial and NASA communications services under study and in development. We explored the communications capabilities driving from the behavior of the astrophysical objects themselves.
title Time-Domain And MultiMessenger Astrophysics Communications Science Analysis Group Report
topic Instrumentation and Methods for Astrophysics
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2410.03980