Указатель цитирования М (стр. 3 )

цитируемый документ

Pitch angle distribution of trapped energetic protons and helium isotope nuclei measured along the Resurs-01 No.4 LEO satellite Author(s): Leonov A, Cyamukungu M, Cabrera J, Leleux P, Lemaire J, Gregorie G, Benck S, Mikhailov V, Bakaldin A, Galper A, Koldashov S, Voronov S, Casolino M, De Pascale M, Picozza P, Sparvolli R, Ricci M Source: ANNALES GEOPHYSICAE Volume: 23 Issue: 9 Pages:  Published: 2005  Times Cited: 1 References: 14  Abstract: The NINA detector on board the Resurs-01 No. 4 satellite (835 kin, 98 degrees inclination) is equipped with particle trackers based on silicon strip detectors. From the energy deposited In each of its silicon layers the mass, the momentum direction and energy of incident particles have been determined. The resolutions in mass and energy allow identification of H and He isotopes over the 10-50MeV/n energy range. The angular resolution is about 2.5 degrees. We present the direct measurements of proton and helium isotopes pitch angle distributions derived from Resurs-01 No.4/NINA observations and their variations as functions of (B, L) coordinates and energy. The measurements of trapped helium isotopes spectrum are also presented. Document Type: Article Language: English Author Keywords: interplanetary physics; cosmic rays; magnetospheric physics; energetic particles, trapped; solar physics, astrophysics and astronomy; instruments and techniques KeyWords Plus: NINA Addresses: Leonov, A (reprint author), Ctr Space Radiat, Chemin Cyclotron 2, B-1348 Louvain, Belgium Ctr Space Radiat, B-1348 Louvain, Belgium Moscow MV Lomonosov State Univ, Moscow Phys Engn Inst, Moscow Russia Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Sez Roma 2, I-00133 Rome, Italy Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy E-mail Addresses: *****@***ru Publisher: EUROPEAN GEOSCIENCES UNION, MAX-PLANCK-STR 13, 37191 KATLENBURG-LINDAU, GERMANY Subject Category: Astronomy & Astrophysics; Geosciences, Multidisciplinary; Meteorology & Atmospheric Sciences IDS Number: 996IE ISSN:

1 цитирование

1. Title: Fluxes of energetic protons and electrons measured on board the Oersted satellite Author(s): Cabrera J, Cyamukungu M, Stauning P, et al. Source: ANNALES GEOPHYSICAE  Volume: 23  Issue: 9  Pages:  Published: 2005 Times Cited: 1

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High-energy charged particle bursts in the near-Earth space as earthquake precursors Author(s): Aleksandrin SY, Galper AM, Grishantzeva LA, Koldashov SV, Maslennikov LV, Murashov AM, Picozza P, Sgrigna V, Voronov SA Source: ANNALES GEOPHYSICAE Volume: 21 Issue: 2 Pages: 597-602 Published: FEB 2003  Times Cited: 3 References: 18  Abstract: The experimental data on high-energy charged particle fluxes, obtained in various near-Earth space experiments (MIR orbital station, METEOR-3, GAMMA and SAMPEX satellites) were processed and analyzed with the goal to search for particle bursts. Particle bursts have been selected in every experiment considered. It was shown that the significant part of high-energy charged particle bursts correlates with seismic activity. Moreover, the particle bursts are observed several hours before strong earthquakes; L-shells of particle bursts and corresponding earthquakes are practically the same. Some features of a seismo-magnetosphere connection model, based on the interaction of electromagnetic emission of seismic origin and radiation belt particles, were considered. Document Type: Article Language: English Author Keywords: ionospheric physics; energetic particles, trapped; energetic particles, precipitating; magnetosphere-ionosphere interactions Addresses: Koldashov, SV (reprint author), Moscow Engn Phys Inst, Space Phys Inst, Kashirskoe Shosse 31, Moscow Russia Moscow Engn Phys Inst, Space Phys Inst, Moscow Russia Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy Ist Nazl Fis Nucl, Sez Roma 2, I-00133 Rome, Italy Univ Rome Roma Tre, Dept Phys, I-00146 Rome, Italy E-mail Addresses: *****@ Publisher: EUROPEAN GEOPHYSICAL SOC, MAX-PLANCK-STR 13, 37191 KATLENBURG-LINDAU, GERMANY Subject Category: Astronomy & Astrophysics; Geosciences, Multidisciplinary; Meteorology & Atmospheric Sciences IDS Number: 775MW ISSN:

3 цитирования

1. Title: Satellite experiment ARINA for studying seismic effects in the high-energy particle fluxes in the earth’s magnetosphere Author(s): Bakaldin AV, Batishchev AG, Voronov SA, et al. Source: COSMIC RESEARCH  Volume: 45  Issue: 5  Pages: 445-448  Published: SEP-OCT 2007 Times Cited: 0 2. Title: Seismo-induced effects in the near-earth space: Combined ground and space investigations as a contribution to earthquake prediction Author(s): Sgrigna V, Buzzi A, Conti L, et al. Source: TECTONOPHYSICS  Volume: 431  Issue: 1-4  Pages: 153-171  Published: FEB Times Cited: 0 3. Title: Correlations between earthquakes and anomalous particle bursts from SAMPEX/PET satellite observations Author(s): Sgrigna V, Carota L, Conti L, et al. Source: JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS  Volume: 67  Issue: 15  Pages:  Published: OCT 2005 Times Cited: 1

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Energy spectrum of secondary protons above the atmosphere measured by the instruments NINA and NINA-2 Author(s): Bidoli V, Casolino M, De Pascale M, Furano G, Iannucci A, Morselli A, Picozza P, Sparvoli R, Bakaldin A, Galper A, Koldashov S, Korotkov M, Leonov A, Mikhailov V, Voronov S, Boezio M, Bonvicini V, Vacchi A, Zampa G, Zampa N, Ambriola M, Cafagna F, Circella M, De Marzo C, Adriani O, Papini P, Spillantini P, Straulino S, Vannuccini E, Ricci M, Castellini G Source: ANNALES GEOPHYSICAE Volume: 20 Issue: 10 Pages:  Published: OCT 2002  Times Cited: 2 References: 14  Abstract: In this paper we report on the energy spectrum of protons of albedo origin measured by the instruments NINA and NINA-2 at different geomagnetic locations, and the behaviour of the proton flux as a function of altitude out of the South Atlantic Anomaly. The instrument NINA was used on board the satellite Resurs-01-N4 between 1998 and 1999, at an altitude of about 830km. The NINA-2 apparatus, on board the satellite MITA, was put into orbit in July 2000, at an altitude of about 450 km. A detailed understanding of the fluxes of charged particles in near Earth orbit is important to reach an accurate theoretical description of the Earth's magnetic field, but also as input for the calculation of the background for scientific instruments aboard satellites, like the future AGILE and GLAST gamma astronomy telescopes. Document Type: Letter Language: English Author Keywords: magnetospheric physics; energetic particles, trapped; instruments and techniques KeyWords Plus: SPACE TELESCOPE NINA; COSMIC-RAY NUCLEI; NEAR-EARTH ORBIT Addresses: Sparvoli, R (reprint author), Univ Roma Tor Vergata, I-00173 Rome, Italy Univ Roma Tor Vergata, I-00173 Rome, Italy Ist Nazl Fis Nucl, Sect Roma2, I-00185 Rome, Italy Moscow Engn Phys Inst, Moscow Russia Univ Trieste, I-34127 Trieste, Italy Ist Nazl Fis Nucl, Sect Trieste, I-34127 Trieste, Italy Univ Bari, I-70126 Bari, Italy Ist Nazl Fis Nucl, Sect Bari, I-70126 Bari, Italy Univ Florence, I-50139 Florence, Italy Ist Nazl Fis Nucl, Sect Florence, I-50125 Florence, Italy Ist Nazl Fis Nucl, Nazl Frascati Lab, I-00044 Frascati, Italy CNR, Inst Appl Phys Nello Carrara, I-50127 Florence, Italy Publisher: EUROPEAN GEOPHYSICAL SOC, MAX-PLANCK-STR 13, 37191 KATLENBURG-LINDAU, GERMANY Subject Category: Astronomy & Astrophysics; Geosciences, Multidisciplinary; Meteorology & Atmospheric Sciences IDS Number: 626AJ ISSN:

1 цитирование (без самоцитирования)

1. Title: Isotope composition of secondary hydrogen and helium above the atmosphere measured by the instruments NINA and NINA-2 Author(s): Bidoli V, Casolino M, De Pascale M, et al. Source: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS  Volume: 108  Issue: A5 Article Number: 1211  Published: MAY Times Cited: 1

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SPECTRAL CHARACTERISTICS OF HIGH-ENERGY GAMMA-RAY SOLAR-FLARES Author(s): LEIKOV NG, AKIMOV VV, VOLZHENSKAYA VA, KALINKIN LF, NESTEROV VE, GALPER AM, ZEMSKOV VM, OSEROV YV, TOPCHIEV NP, FRADKIN MI, TCHUIKIN EI, TUGAENKO VY, GROS M, GRENIER I, BAZERBACHI AR, LAVIGNE JM, OLIVE JF Source: ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES Volume: 97 Issue: 1 Pages: 345-348 Published: JAN 1993  Times Cited: 10 References: 9  Abstract: The gamma-ray telescope GAMMA-1 has registered gamma-emission in the range 30-2000 MeV from two solar flares. Spectral analysis with the use of maximum likelihood and maximum entropy methods has revealed differences in gamma-ray production mechanisms. In the impulsive March 26, 1991 event high energy gamma-rays originate exclusively as a bremsstrahlung of primary accelerated electrons. In contrast, the gamma ray emission of the extended phase of June 15, 1991 flare is mainly due to the decay of neutral pions. The average spectral index for primary nucleons was -3.6. Evolution of the spectra for both flares shows tendency to a decrease of the primary particles mean energies with time. Document Type: Article Language: English Author Keywords: SOLAR FLARES; GAMMA-RAY; DATA ANALYSIS KeyWords Plus: TELESCOPE GAMMA-1 Addresses: LEIKOV, NG (reprint author), ACAD SCI RF, SPACE RES INST, PROFSOYUZNAYA 84-32, MOSCOW RUSSIA MOSCOW PHYS ENGN INST, MOSCOW RUSSIA PN LEBEDEV PHYS INST, MOSCOW RUSSIA AF IOFFE PHYS & TECH, ST PETERSBURG RUSSIA NPO ENERGIA, KALININGRAD, RUSSIA CENS, F-91191 GIF SUR YVETTE, FRANCE CTR ETUD SPATIALE RAYONNEMENTS, F-31029 TOULOUSE, FRANCE Publisher: EDITIONS PHYSIQUE, Z I DE COURTABOEUF AVE 7 AV DU HOGGAR, BP 112, 91944 LES ULIS CEDEX, FRANCE Subject Category: Astronomy & Astrophysics IDS Number: KJ736 ISSN:

10 цитирований

1. Title: Nuclear deexcitation gamma-ray lines from accelerated particle interactions Author(s): Kozlovsky B, Murphy RJ, Ramaty R Source: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES  Volume: 141  Issue: 2  Pages: 523-541  Published: AUG 2002 Times Cited: 18 2. Title: First detection of the impulsive and extended phases of a solar radio burst above 200 GHz Author(s): Trottet G, Raulin JP, Kaufmann P, et al. Source: ASTRONOMY & ASTROPHYSICS  Volume: 381  Issue: 2  Pages: 694-702  Published: JAN 2002 Times Cited: 14 3. Title: Flare-associated energetic particles in the corona and at 1 AU Author(s): Klein KL, Chupp EL, Trottet G, et al. Source: ASTRONOMY AND ASTROPHYSICS  Volume: 348  Issue: 1  Pages: 271-285  Published: AUG 1999 Times Cited: 22 4. Title: Electrons and gamma rays from near-solar supersymmetric dark matter annihilations Author(s): Strausz SC Source: PHYSICAL REVIEW D  Volume: 59  Issue: 12 Article Number: 123514  Published: JUN Times Cited: 0 5. Title: Hard X-ray and gamma-ray observations of an electron dominated event associated with an occulted solar flare Author(s): Vilmer N, Trottet G, Barat C, et al. Source: ASTRONOMY & ASTROPHYSICS  Volume: 342  Issue: 2  Pages: 575-582  Published: FEB 1999 Times Cited: 13 6. Title: Search for energetic cosmic axions utilizing terrestrial/celestial magnetic fields Author(s): Zioutas K, Thompson DJ, Paschos EA Source: PHYSICS LETTERS B  Volume: 443  Issue: 1-4  Pages: 201-208  Published: DEC Times Cited: 2 7. Title: Evidence for prolonged acceleration based on a detailed analysis of the long-duration solar gamma-ray flare of June 15, 1991 Author(s): Akimov VV, Ambroz P, Belov AV, et al. Source: SOLAR PHYSICS  Volume: 166  Issue: 1  Pages: 107-134  Published: JUN 1996 Times Cited: 36 8. Title: ON A ROLE OF CORONAL MASS ELECTIONS IN SOLAR-FLARE EVENTS Author(s): CHERTOK IM Source: IZVESTIYA AKADEMII NAUK SERIYA FIZICHESKAYA  Volume: 59  Issue: 7  Pages: 112-123  Published: JUL 1995 Times Cited: 2 9. Title: NEUTRON MONITOR DATA ON THE 15 JUNE 1991 FLARE - NEUTRONS AS A TEST FOR PROTON ACCELERATION SCENARIO Author(s): KOVALTSOV GA, USOSKIN IG, KOCHAROV LG, et al. Source: SOLAR PHYSICS  Volume: 158  Issue: 2  Pages: 395-398  Published: MAY 1995 Times Cited: 2 10. Title: SOLAR HARD X-RAY AND GAMMA-RAY OBSERVATIONS FROM GRANAT Author(s): VILMER N Source: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES  Volume: 90  Issue: 2  Pages: 611-621  Published: FEB 1994 Times Cited: 10

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OBSERVATION OF THE VELA GAMMA-RAY PULSAR WITH THE GAMMA-1 TELESCOPE Author(s): OLIVE JF, LEIKOV N, AKIMOV V, AFANASSYEV V, BAROUCH E, BAZERBACHI R, BLOCHINTSEV I, BUCZKOWSKA A, CHUIKIN E, FRADKIN M, GALPER A, GRENIER I, GROS M, GRYGORCZUK J, JUCHNIEWICZ J, LAVIGNE JM, MCCULLOCH P, NESTEROV V, OZEROV Y, RUDKO V, TOPCHIEV N, ZEMSKOV V Source: ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES Volume: 97 Issue: 1 Pages: 325-327 Published: JAN 1993  Times Cited: 1 References: 8  Abstract: The GAMMA-1 telescope observed PSR0833-45 in the summer of 1990 and spring of 1991. We found that the mean MeV flux (5.25 +/- 0.45 x 10(-6) ph/cm2 sec) of the whole pulsed emission is consistent with the time-averaged COS-B result (). The 50-300 MeV flux (8.30 +/- 2.9 x 10(-6) ph/cm2 sec) suggests that we observed the pulsar in a low intensity state. The emission from the first peak appears softer than the second peak (first observation: 1.7sigma, second: 3sigma confidence level). We investigate the variation of the spectra with time. Document Type: Article Language: English Author Keywords: GAMMA-RAYS, PULSARS; PSR0833-45, VELA Addresses: OLIVE, JF (reprint author), CTR ETUD SPATIALE RAYONNEMENTS, 9 AVE COLONEL ROCHE, BP4346, F-31029 TOULOUSE, FRANCE ACAD SCI, SPACE RES INST, MOSCOW RUSSIA AF IOFFE PHYS & TECH INST, ST PETERSBURG, RUSSIA CENS, CEA, SERV ASTROPHYS, F-91191 GIF SUR YVETTE, FRANCE PN LEBEDEV PHYS INST, MOSCOW, RUSSIA POLISH ACAD SCI, CBK, WARSAW, POLAND MOSCOW ENGN PHYS INST, MOSCOW, RUSSIA UNIV TASMANIA, DEPT PHYS, HOBART, TAS 7001 AUSTRALIA Publisher: EDITIONS PHYSIQUE, Z I DE COURTABOEUF AVE 7 AV DU HOGGAR, BP 112, 91944 LES ULIS CEDEX, FRANCE Subject Category: Astronomy & Astrophysics IDS Number: KJ736 ISSN:

1 цитирование

1. Title: EGRET OBSERVATIONS OF THE VELA PULSAR, PSR0833-45 Author(s): KANBACH G, ARZOUMANIAN Z, BERTSCH DL, et al. Source: ASTRONOMY AND ASTROPHYSICS  Volume: 289  Issue: 3  Pages: 855-867  Published: SEP Times Cited: 81

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Spatial correlation of unidentified gamma-ray sources with flaring and Wolf-Rayet stars Author(s): Galper AM, Luchkov BI Source: ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS Volume: 30 Issue: 6 Pages: 390-392 Published: JUN 2004  Times Cited: 1 References: 7  Abstract: The spatial positions of unidentified gamma-ray sources (E > 100 MeV) were analyzed. This analysis shows that gamma-ray sources with fluxes >5 x 10(-7) cm(-2) s(-1) correlate with Wolf-Rayet stars, while gamma-ray sources with fluxes <5 x 10(-7) cm(-2) s(-1) may be associated with flaring stars. (C) 2004 MAIK "Nauka/Interperiodica". Document Type: Article Language: English Author Keywords: unidentified gamma-ray sources; flaring stars; Wolf-Rayet stars KeyWords Plus: CATALOG Addresses: Galper, AM (reprint author), Moscow Engn Phys Inst, Kashirskoe 31, Moscow Russia Moscow Engn Phys Inst, Moscow Russia E-mail Addresses: *****@ Publisher: MAIK NAUKA/INTERPERIODICA PUBL, C/O AMERICAN INST PHYSICS, 2 HUNTINGTON QUANDRANGLE, STE 1NO1, MELVILLE, NY USA Subject Category: Astronomy & Astrophysics IDS Number: 833WB ISSN:

1 цитирование

1. Title: Astrophysics in 2004 Author(s): Trimble V, Aschwanden M Source: PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC  Volume: 117  Issue: 830  Pages: 311-394  Published: APR 2005 Times Cited: 1

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THE LIGHT-CURVE OF THE GEMINGA GAMMA-RAY PULSAR AT MEV ACCORDING TO GAMMA-1 TELESCOPE DATA Author(s): AKIMOV VV, AFANASEV VG, BLOKHINTSEV ID, KALINKIN LF, LEIKOV NG, NESTEROV VE, GALPER AM, OZEROV YV, RUDKO VA, RUNTSO MF, ZEMSKOV VM, KURNOSOVA LV, RUSAKOVICH MA, TOPCHIEV NP, FRADKIN MI, CHUIKIN EI, TUGAENKO VY, GROS M, GRENIER I, BAZERBACHI AR, LAVIGNE JM, OLIVE JF Source: ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS Volume: 19 Issue: 4 Pages: 229-230 Published: JUL-AUG 1993  Times Cited: 3 References: 8  Abstract: Using Gamma 1 telescope data, we obtained the light curve of Geminga, with two peaks separated by 0.5 +/- 0.03 of the period. The light curve is clearly defined for gamma energies above 400 MeV. The upper limit (1sigma) of the pulsed flux for energies 50-300 MeV equals cm-2 sec 1. For energies above 300 MeV, the spectral index of the pulsed component is 1.1 (+ 1.1/-0.3), and the integrated flux equals (1.1 +/- 0cm-2 sec-1. Document Type: Article Language: English Addresses: AKIMOV, VV (reprint author), RUSSIAN ACAD SCI, SPACE RES INST, MOSCOW, RUSSIA MOSCOW ENGN PHYS INST, MOSCOW, RUSSIA RUSSIAN ACAD SCI, INST PHYS, MOSCOW, RUSSIA RUSSIAN ACAD SCI, INST TECH PHYS, ST PETERSBURG, RUSSIA ENERGIYA SCI IND ASSOC, KALININGRAD, RUSSIA CEN, SACLAY, FRANCE CTR ETUD SPATIALE RAYONNEMENTS, TOULOUSE, FRANCE Publisher: AMER INST PHYSICS, CIRCULATION FULFILLMENT DIV, 500 SUNNYSIDE BLVD, WOODBURY, NY Subject Category: Astronomy & Astrophysics IDS Number: MT259 ISSN:

3 цитирования

1. Title: A 59-second period in the very high energy gamma-ray emission from the geminga pulsar Author(s): Neshpor YI, Stepanyan AA Source: ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS  Volume: 27  Issue: 12  Pages: 794-798  Published: DEC 2001 Times Cited: 2 2. Title: Ultrahigh-energy gamma-ray emission from the Geminga pulsar Author(s): Neshpor YI, Stepanyan AA, Zyskin YL, et al. Source: ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS  Volume: 27  Issue: 4  Pages: 228-232  Published: APR 2001 Times Cited: 2 3. Title: Geminga: Its phenomenology, its fraternity, and its physics Author(s): Bignami GF, Caraveo PA Source: ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS  Volume: 34  Pages: 331-381  Published: 1996 Times Cited: 44

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