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GF37688754

Carbon

foil, 25x25mm, thickness 0.5mm, rigid graphite, fine grain size, 99.997%

Synonym(s):

Activated charcoal, C 000421, Charcoal activated

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About This Item

Empirical Formula (Hill Notation):
C
CAS Number:
7440-44-0
Molecular Weight:
12.01
MDL number:
MFCD00133992
UNSPSC Code:
12141908
PubChem Substance ID:
329805722
NACRES:
NA.23

vapor pressure

<0.1 mmHg ( 20 °C)

Assay

99.997%

form

foil

autoignition temp.

842 °F

manufacturer/tradename

Goodfellow 376-887-54

resistivity

1375 μΩ-cm, 20°C (graphite)

size × thickness

25 × 25 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

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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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