Event calendar file
3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
SH 3.4, SH 3.5
Place
Location: Merida, Mexico
Room: Yucatan I (Fiesta Americana)
Date:
10 Jul 08:30 - 10:00
Conveners
-
- Dr. Kota, Jozsef (University of Arizona)
Timetable | Contribution List
Displaying 7
contributions
out of
7
The propagation of galactic and solar cosmic rays in the
solar wind (SW) can be strongly influenced by the SW
fluctuations properties. Magnetohydrodynamic (MHD) scale
fluctuations in the solar wind are usually highly
anisotropic, and have also been found to exhibit different
properties in regions of high and low solar wind speed.
We analyze here the anisotropy properties of the solar
wind f
... More
Presented by Dr. Sergio DASSO
on
10/7/2007
at
14:18
Energetic heavy ions with 20 – 200 MeV/n in the radiation belts have been observed by
Heavy Ion Telescope (HIT) onboard TSUBASA satellite which stayed in the geostationary
transfer orbit with the inclination of 28.5 deg. The observed data during quiet
period in the outer region of radiation belt found out that the relative abundance
for major elements, C, O, Ne, Mg, Si and Fe, were similar t
... More
Presented by Dr. Makoto HAREYAMA
on
10/7/2007
at
14:42
We present preliminary results of measuring the direction of the anisotropy
vector of cosmic ray intensity. The measurements were made with the Carpet
air shower array of the Baksan Neutrino Observatory. The anisotropy vector
direction is determined by analyzing the distribution of time delays of the
shower signal detected by distant detectors of the array relative to the array’s
centr
... More
Presented by Dr. Alexander LIDVANSKY
on
10/7/2007
at
13:42
This paper presents the sidereal anisotropy of ~10 TeV galactic cosmic ray
(GCR) intensity observed by the Tibet Air Shower experiment. The observed sky-
map of the directional anisotropy clearly shows the large-scale feature
consisting of excess and deficit of the relative intensity. We note that the
observed angular separation between the excess and the deficit is ~120 deg,
which is muc
... More
Presented by Prof. M. TAKITA
on
10/7/2007
at
13:30
The relative sidereal variation in the arrival direction of primary
cosmic ray nuclei of median energy 10 TeV was measured using downward,
through-going muons detected with the Super-Kamiokande-I detector.
The projection of the anisotropy map onto the right ascension axis has
a first harmonic amplitude of
(6.64 +/- 0.98 (stat.) +/- 0.55 (syst.)) x 10^-4 and a phase at maximum at
(33.2^o +/-
... More
Presented by Dr. Yuichi OYAMA
on
10/7/2007
at
13:54
PAMELA was launched on June $15^{th}$ 2006 in a pressurized container on board the
Russian Resurs-DK1 satellite. The satellite is flying in high inclination ($70^o$),
low Earth Orbit (350-600 km), allowing measurements in various points and
conditions of the geomagnetosphere. It is a multi-purpose apparatus composed of a
permanent
magnet spectrometer to provide particle charge, rig
... More
Presented by Dr. Marco CASOLINO
on
10/7/2007
at
14:30
On the basis of world network data of neutron monitors and muon telescopes
at the Yakutsk and Nagoya stations the galactic cosmic ray anisotropy directed
transverse to the mean field line (in the direction of 15.00 LT) has been
revealed. This component undergoes the 11-year variation. Its value rises as
the IMF intensity, solar activity level and neutral sheet deformation increase.
Such
... More
Presented by Dr. Sardaana GERASIMOVA
on
10/7/2007
at
14:06
