揮發性分子在低溫固化夏之能量作用機制研究II(1/3)

Keyphrases

1. Ice Analogs 100%
2. X-ray 100%
3. Photodesorption 100%
4. Gas Enrichment 66%
5. Circumstellar 66%
6. Desorption Yield 40%
7. Low Temperature 33%
8. Formation Mechanism 33%
9. Volatile Molecules 33%
10. Solid Phase 33%
11. Energetic Processes 33%
12. Absorbed Photons 26%
13. Weakly Bound 26%
14. Pluto 16%
15. Extreme Ultraviolet 16%
16. Interstellar Ice 16%
17. Ultraviolet Rays 16%
18. Astrophysical Ices 16%
19. Vacuum Ultraviolet 16%
20. Organic Molecules 16%
21. Surface Techniques 16%
22. Gas Chromatography-mass Spectrometry 16%
23. Interstellar Chemistry 16%
24. Polar Ice 16%
25. Physics Chemistry 16%
26. Secondary Electron 16%
27. Ultra-high Vacuum 16%
28. Mass Spectrometry 16%
29. High-performance Liquid Chromatography 16%
30. Yield Decline 13%
31. Species Decline 13%
32. Complex Species 13%
33. Disc Model 13%
34. Taiwan 13%
35. Order of Magnitude 13%
36. Porosity Effect 13%
37. Surface-to-volume Ratio 13%
38. Synchrotron Radiation 13%
39. Desorption 13%
40. Gas Phase 13%
41. Hsinchu 13%
42. Soft X-ray 13%
43. T Tauri Stars 13%
44. Atomic Hydrogen 13%
45. Radiation Research 13%
46. Exciton 13%
47. Substrate-mediated 13%
48. Protoplanetary Disks 13%

Physics

1. Desorption 66%
2. Vapor Phase 66%
3. Mass Spectroscopy 33%
4. Energetics 33%
5. X Ray 33%
6. Interstellar Molecules 16%
7. Ultrahigh Vacuum 16%
8. Physics 16%
9. Interstellar Chemistry 16%
10. T Tauri Stars 11%
11. Protoplanetary Disk 11%
12. Exciton 11%
13. Synchrotron Radiation 11%
14. Porosity 11%