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Fail:Helium atom QM.png

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Ringkasan

Keterangan A semi-accurate depiction of the helium atom. The darkness of the electron cloud corresponds to the line-of-sight integral over the probability function of the 1s electron orbital. The magnified nucleus is schematic, showing protons in pink and neutrons in purple. In reality, the nucleus is also spherically symmetric.
Tarikh
Sumber http://en.wikipedia.org/wiki/Image:Helium_atom_QM.png
Pengarang en:User:FrankH
Kebenaran
(Penggunaan semula fail ini)

"I, the creator of this work, hereby release it into the public domain. This applies worldwide. In case this is not legally possible,

I grant any entity the right to use this work for any purpose, without any conditions, unless such conditions are required by law."

Perlesenan

Public domain Xerxes314 at Inggeris Wikipedia selaku pemegang hak cipta karya ini melepaskan karya ini ke dalam domain awam di seluruh dunia.
Di sesetengah negara, undang-undangnya mungkin tidak mengizinkan; jika begitu:
Xerxes314 memberi sesiapa sahaja hak untuk menggunakan karya ini untuk apa jua tujuan, tanpa sebarang syarat, melainkan undang-undang menetapkan syarat-syarat sedemikian.

History

  • (Delete all revisions of this file) (cur) 09:31, 21 September 2006 . . FrankH (Talk | contribs | block) . . 625×625 (47,274 bytes) (Second try - previous attempt did not seem to actually get uploaded. Same comment as previous edit.)
  • (del) (rev) 09:10, 21 September 2006 . . FrankH (Talk | contribs | block) . . 625×625 (47,274 bytes) (I made some edits to the excellent image from Xerxes314 - I shadowed the black lines with white lines so they would not get lost in the black electron cloud and I added text to quickly remind users of the tremendous change in scale for the nucleus inset i)
  • (del) (rev) 00:31, 12 May 2006 . . Xerxes314 (Talk | contribs | block) . . 625×625 (45,147 bytes)
  • (del) (rev) 00:25, 12 May 2006 . . Xerxes314 (Talk | contribs | block) . . 625×625 (45,181 bytes)
  • (del) (rev) 20:59, 11 May 2006 . . Bensaccount (Talk | contribs | block) . . 400×400 (33,507 bytes) (Reverted to earlier revision)
  • (del) (rev) 20:59, 11 May 2006 . . Bensaccount (Talk | contribs | block) . . 400×400 (38,065 bytes) (Reverted to earlier revision)
  • (del) (rev) 21:49, 10 February 2006 . . Xerxes314 (Talk | contribs | block) . . 400×400 (40,110 bytes)
  • (del) (rev) 21:27, 10 February 2006 . . Xerxes314 (Talk | contribs | block) . . 400×400 (38,065 bytes)
  • (del) (rev) 23:09, 7 February 2006 . . Xerxes314 (Talk | contribs | block) . . 400×400 (33,507 bytes) (A semi-accurate depiction of the helium atom. The darkness of the electron cloud corresponds to the line-of-sight integral over the probability function of the 1s electron orbital. The magnified nucleus is schematic,)

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21 September 2006

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semasa21:49, 31 Oktober 2006Gambar kenit bagi versi pada 21:49, 31 Oktober 2006625 × 625 (46 KB)InfoCan{{Information |Description=A semi-accurate depiction of the helium atom. The darkness of the electron cloud corresponds to the line-of-sight integral over the probability function of the 1s electron orbital. The magnified nucleus is schematic, showing pro

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