GF95501729
Carbon
foil, 50x50mm, thickness 0.5mm, rigid graphite, fine grain size, 99.95%
Synonym(s):
Activated charcoal, C 000420, Charcoal activated
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About This Item
Empirical Formula (Hill Notation):
C
CAS Number:
Molecular Weight:
12.01
MDL number:
UNSPSC Code:
12141908
PubChem Substance ID:
NACRES:
NA.23
vapor pressure
<0.1 mmHg ( 20 °C)
Assay
≥99.95%
form
foil
autoignition temp.
842 °F
manufacturer/tradename
Goodfellow 955-017-29
resistivity
1375 μΩ-cm, 20°C (graphite)
size × thickness
50 × 50 mm × 0.5 mm
mp
3550 °C (lit.)
SMILES string
[C]
InChI
1S/C
InChI key
OKTJSMMVPCPJKN-UHFFFAOYSA-N
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General description
For updated SDS information please visit www.goodfellow.com.
Legal Information
Product of Goodfellow
Storage Class Code
13 - Non Combustible Solids
WGK
nwg
Flash Point(F)
Not applicable
Flash Point(C)
Not applicable
Regulatory Information
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Investigation of delta -electron emission in collisions of highly charged fast Ne projectiles with carbon-foil targets.
Schiwietz et al.
Physical review. B, Condensed matter, 41(10), 6262-6271 (1990-04-01)
I Dietrich et al.
Ultramicroscopy, 3(2), 185-189 (1978-01-01)
Radiation damage on a holey carbon foil was investigated in an electron microscope with a superconducting lens system, where the temperature of the specimen and its environment initially was 4 K. Due to an electron dose of 2 X 10(4)
Doubly differential secondary-electron yields following 8-MeV/u U68+- and 3.5-MeV/u U38+-ion impact on a thin carbon-foil target.
Schneider et al.
Physical review. A, Atomic, molecular, and optical physics, 47(5), 3945-3950 (1993-05-01)
Systematics of equilibrium charge distributions of ions passing through a carbon foil over the ranges Z=4-92 and E=0.02-6 MeV/u.
Shima et al.
Physical review. A, General physics, 40(7), 3557-3570 (1989-10-01)
D J McComas et al.
Proceedings of the National Academy of Sciences of the United States of America, 88(21), 9598-9602 (1991-11-01)
Global imaging of the magnetospheric charged particle population can be achieved by remote measurement of the neutral atoms produced when magnetospheric ions undergo charge exchange with cold exospheric neutral atoms. Previously suggested energetic neutral atom imagers were only able to
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