Cosmic Ray Energetics And Mass (CREAM)

  • Increase font size
  • Default font size
  • Decrease font size

CREAM Mission Overview

E-mail Print PDF
CREAM Members The Cosmic Ray Energetics and Mass (CREAM) experiment was designed and constructed to measure cosmic ray elemental spectra using a series of ultra long duration balloon (ULDB) flights. The goal is to extend direct measurement of cosmic-ray composition to the energies capable of generating gigantic air showers which have been mainly observed on the ground, thereby providing calibration for indirect measurements. The instrument has redundant and complementary charge identification and energy measurement systems capable of precise measurements of elemental spectra for Z = 1 - 26 nuclei over the energy range ~1011 to 1015 eV. Precise measurements of the energy dependance of elemetal spectra at the highest of these energies, where the rigidity-dependant supernova acceleration limit could be reflected in a composition change, provide a key to understanding cosmic ray acceleration and propogation. The instrument includes a Timing Charge Detector (TCD), a Cherankov Detector (CD), a Transition Radiation Detector (TRD), a Cherenkov Camera (CherCam), a Silicon Charge Detector (SCD), scintillating fiber hodoscopes, and a tungsten-scintillating fiber calorimeter.

The CREAM mission has had four successful flights: (1) 12/16/04 – 1/27/05, (2) 12/16/05 – 1/13/06, (3) 12/19/07 – 1/17/08, and (4) 12/19/08 – 1/7/09, respectively called CREAM-I, -II, -III, and -IV. A 40 million cubic foot (1.1 million cubic meter) balloon carried each payload to its float altitude between ~38 and ~40 km, with an average atmospheric overburden of ~3.9 g/cm2. A cumulative exposure of 119 days has been achieved.
Last Updated on Wednesday, 04 November 2009 18:34
 

Official CREAM Logo

CREAM Logo

CREAM IV Flight Trajectory

Click the map below to see the CREAM IV flight trajectory.

CREAM IV Flight Trajectory

Who's Online

We have 25 guests online

Statistics

Content View Hits : 27564