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Sökning: onr:"swepub:oai:DiVA.org:kth-273509" > Time Dependence of ...
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 03114naa a2200397 4500 | |
| 001 | oai:DiVA.org:kth-273509 | |
| 003 | SwePub | |
| 008 | 200525s2020 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2735092 URI |
| 024 | 7 | a https://doi.org/10.3847/1538-4357/ab80c22 DOI |
| 040 | a (SwePub)kth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Marcelli, N.u Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy.;INFN, Sez Rome Tor Vergata, I-00133 Rome, Italy.4 aut |
| 245 | 1 0 | a Time Dependence of the Flux of Helium Nuclei in Cosmic Rays Measured by the PAMELA Experiment between 2006 July and 2009 December |
| 264 | c 2020-04-24 | |
| 264 | 1 | b IOP PUBLISHING LTD,c 2020 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20200525 | |
| 520 | a Precise time-dependent measurements of the Z = 2 component in the cosmic radiation provide crucial information about the propagation of charged particles through the heliosphere. The PAMELA experiment, with its long flight duration (2006 June 15-2016 January 23) and the low energy threshold (80 MeV/n) is an ideal detector for cosmic-ray solar modulation studies. In this paper, the helium nuclei spectra measured by the PAMELA instrument from 2006 July to 2009 December over a Carrington rotation time basis are presented. A state-of-the-art three-dimensional model for cosmic-ray propagation inside the heliosphere was used to interpret the time-dependent measured fluxes. Proton-to-helium flux ratio time profiles at various rigidities are also presented in order to study any features that could result from the different masses and local interstellar spectra shapes. | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a Cosmic ray detectors | |
| 653 | a Galactic cosmic rays | |
| 653 | a Heliosphere | |
| 700 | 1 | a Munini, R.u INFN, Sez Trieste, I-34149 Trieste, Italy.;IFPU, I-34014 Trieste, Italy.4 aut |
| 700 | 1 | a Carlson, Peru KTH,Partikel- och astropartikelfysik,Albanova VinnExcellence Center for Protein Technology, ProNova,Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden.4 aut0 (Swepub:kth)u1ua4u32 |
| 700 | 1 | a Pearce, Mark,d 1970-u KTH,Partikel- och astropartikelfysik,Albanova VinnExcellence Center for Protein Technology, ProNova,Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden.4 aut0 (Swepub:kth)u17jptna |
| 700 | 1 | a Zampa, N.u INFN, Sez Trieste, I-34149 Trieste, Italy.4 aut |
| 710 | 2 | a Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy.;INFN, Sez Rome Tor Vergata, I-00133 Rome, Italy.b INFN, Sez Trieste, I-34149 Trieste, Italy.;IFPU, I-34014 Trieste, Italy.4 org |
| 773 | 0 | t Astrophysical Journald : IOP PUBLISHING LTDg 893:2q 893:2x 0004-637Xx 1538-4357 |
| 856 | 4 | u https://iopscience.iop.org/article/10.3847/1538-4357/ab80c2/pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-273509 |
| 856 | 4 8 | u https://doi.org/10.3847/1538-4357/ab80c2 |
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