The status and future of the third interplanetary network

K. Hurley; T. Cline; I. G. Mitrofanov; D. Golovin; M. L. Litvak; A. B. Sanin; W. Boynton; C. Fellows; K. Harshman; R. Starr; S. Golenetskii; R. Aptekar; E. Mazets; V. Pal'shin; D. Frederiks; D. M. Smith; C. Wigger; W. Hajdas; A. Zehnder; A. Von Kienlin; G. G. Lichti; A. Rau; K. Yamaoka; M. Ohno; Y. Fukazawa; T. Takahashi; M. Tashiro; Y. Terada; T. Murakami; K. Makishima; S. Barthelmy; J. Cummings; N. Gehrels; H. Krimm; J. Goldsten; E. Del Monte; M. Feroci; M. Marisaldi

doi:10.1063/1.3155966

The status and future of the third interplanetary network

K. Hurley, T. Cline, I. G. Mitrofanov, D. Golovin, M. L. Litvak, A. B. Sanin, W. Boynton, C. Fellows, K. Harshman, R. Starr, S. Golenetskii, R. Aptekar, E. Mazets, V. Pal'shin, D. Frederiks, D. M. Smith, C. Wigger, W. Hajdas, A. Zehnder, A. Von KienlinG. G. Lichti, A. Rau, K. Yamaoka, M. Ohno, Y. Fukazawa, T. Takahashi, M. Tashiro, Y. Terada, T. Murakami, K. Makishima, S. Barthelmy, J. Cummings, N. Gehrels, H. Krimm, J. Goldsten, E. Del Monte, M. Feroci, M. Marisaldi

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

4 Scopus citations

Abstract

The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds; Wind, up to ∼7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. Ulysses and HETE have ceased operations, and the Fermi GBM is being incorporated into the network. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6x10^-7 erg cm^-2 or 1 photon cm^-2 s ^-1. It detects about 275 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view imaging instruments such as Swift, INTEGRAL IBIS, and SuperAGILE; the localization accuracy is in the several arcminute and above range.

Original language	English (US)
Title of host publication	Gamma-Ray Burst - 6th Huntsville Symposium
Pages	55-57
Number of pages	3
DOIs	https://doi.org/10.1063/1.3155966
State	Published - 2009
Externally published	Yes
Event	6th Huntsville Symposium on Gamma-Ray Bursts - Huntsville, AL, United States Duration: Oct 20 2008 → Oct 23 2008

Publication series

Name	AIP Conference Proceedings
Volume	1133
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	6th Huntsville Symposium on Gamma-Ray Bursts
Country/Territory	United States
City	Huntsville, AL
Period	10/20/08 → 10/23/08

Keywords

Gamma-rays: Bursts
Instrumentation: Detectors

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1063/1.3155966

Cite this

Hurley, K., Cline, T., Mitrofanov, I. G., Golovin, D., Litvak, M. L., Sanin, A. B., Boynton, W., Fellows, C., Harshman, K., Starr, R., Golenetskii, S., Aptekar, R., Mazets, E., Pal'shin, V., Frederiks, D., Smith, D. M., Wigger, C., Hajdas, W., Zehnder, A., ... Marisaldi, M. (2009). The status and future of the third interplanetary network. In Gamma-Ray Burst - 6th Huntsville Symposium (pp. 55-57). (AIP Conference Proceedings; Vol. 1133). https://doi.org/10.1063/1.3155966

Hurley, K, Cline, T, Mitrofanov, IG, Golovin, D, Litvak, ML, Sanin, AB, Boynton, W, Fellows, C, Harshman, K, Starr, R, Golenetskii, S, Aptekar, R, Mazets, E, Pal'shin, V, Frederiks, D, Smith, DM, Wigger, C, Hajdas, W, Zehnder, A, Von Kienlin, A, Lichti, GG, Rau, A, Yamaoka, K, Ohno, M, Fukazawa, Y, Takahashi, T, Tashiro, M, Terada, Y, Murakami, T, Makishima, K, Barthelmy, S, Cummings, J, Gehrels, N, Krimm, H, Goldsten, J, Del Monte, E, Feroci, M & Marisaldi, M 2009, The status and future of the third interplanetary network. in Gamma-Ray Burst - 6th Huntsville Symposium. AIP Conference Proceedings, vol. 1133, pp. 55-57, 6th Huntsville Symposium on Gamma-Ray Bursts, Huntsville, AL, United States, 10/20/08. https://doi.org/10.1063/1.3155966

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title = "The status and future of the third interplanetary network",

abstract = "The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds; Wind, up to ∼7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. Ulysses and HETE have ceased operations, and the Fermi GBM is being incorporated into the network. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6x10-7 erg cm-2 or 1 photon cm-2 s -1. It detects about 275 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view imaging instruments such as Swift, INTEGRAL IBIS, and SuperAGILE; the localization accuracy is in the several arcminute and above range.",

keywords = "Gamma-rays: Bursts, Instrumentation: Detectors",

author = "K. Hurley and T. Cline and Mitrofanov, {I. G.} and D. Golovin and Litvak, {M. L.} and Sanin, {A. B.} and W. Boynton and C. Fellows and K. Harshman and R. Starr and S. Golenetskii and R. Aptekar and E. Mazets and V. Pal'shin and D. Frederiks and Smith, {D. M.} and C. Wigger and W. Hajdas and A. Zehnder and {Von Kienlin}, A. and Lichti, {G. G.} and A. Rau and K. Yamaoka and M. Ohno and Y. Fukazawa and T. Takahashi and M. Tashiro and Y. Terada and T. Murakami and K. Makishima and S. Barthelmy and J. Cummings and N. Gehrels and H. Krimm and J. Goldsten and {Del Monte}, E. and M. Feroci and M. Marisaldi",

year = "2009",

doi = "10.1063/1.3155966",

language = "English (US)",

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series = "AIP Conference Proceedings",

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T1 - The status and future of the third interplanetary network

AU - Hurley, K.

AU - Cline, T.

AU - Mitrofanov, I. G.

AU - Golovin, D.

AU - Litvak, M. L.

AU - Sanin, A. B.

AU - Boynton, W.

AU - Fellows, C.

AU - Harshman, K.

AU - Starr, R.

AU - Golenetskii, S.

AU - Aptekar, R.

AU - Mazets, E.

AU - Pal'shin, V.

AU - Frederiks, D.

AU - Smith, D. M.

AU - Wigger, C.

AU - Hajdas, W.

AU - Zehnder, A.

AU - Von Kienlin, A.

AU - Lichti, G. G.

AU - Rau, A.

AU - Yamaoka, K.

AU - Ohno, M.

AU - Fukazawa, Y.

AU - Takahashi, T.

AU - Tashiro, M.

AU - Terada, Y.

AU - Murakami, T.

AU - Makishima, K.

AU - Barthelmy, S.

AU - Cummings, J.

AU - Gehrels, N.

AU - Krimm, H.

AU - Goldsten, J.

AU - Del Monte, E.

AU - Feroci, M.

AU - Marisaldi, M.

PY - 2009

Y1 - 2009

N2 - The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds; Wind, up to ∼7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. Ulysses and HETE have ceased operations, and the Fermi GBM is being incorporated into the network. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6x10-7 erg cm-2 or 1 photon cm-2 s -1. It detects about 275 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view imaging instruments such as Swift, INTEGRAL IBIS, and SuperAGILE; the localization accuracy is in the several arcminute and above range.

AB - The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds; Wind, up to ∼7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. Ulysses and HETE have ceased operations, and the Fermi GBM is being incorporated into the network. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6x10-7 erg cm-2 or 1 photon cm-2 s -1. It detects about 275 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view imaging instruments such as Swift, INTEGRAL IBIS, and SuperAGILE; the localization accuracy is in the several arcminute and above range.

KW - Gamma-rays: Bursts

KW - Instrumentation: Detectors

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DO - 10.1063/1.3155966

M3 - Conference contribution

AN - SCOPUS:70450181998

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T3 - AIP Conference Proceedings

SP - 55

EP - 57

BT - Gamma-Ray Burst - 6th Huntsville Symposium

T2 - 6th Huntsville Symposium on Gamma-Ray Bursts

Y2 - 20 October 2008 through 23 October 2008

ER -

The status and future of the third interplanetary network

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Keywords

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