1 / 27

Cosmic Brownies

Cosmic Brownies. Attack of the Demon Sun. Not To Scale. 1.5*10 8 km. 0.56m. 2.9m. 2.9m. Φ = π -2 ϴ. ϴ = tan -1 (2.9/.56) = 1.38 rad. Φ = 0.38 rad. Φ. 2.9m. ϴ ϴ. 0.56 m. ϴ = 1.38 rad. Φ = 0.38 rad. Night Fall @ 18:30. Day Break @ 5:30. 0 .38*780 π. 11:13 – 12:47.

makya
Download Presentation

Cosmic Brownies

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Cosmic Brownies Attack of the Demon Sun

  2. Not To Scale 1.5*108 km

  3. 0.56m 2.9m 2.9m

  4. Φ = π-2ϴ ϴ = tan-1(2.9/.56) = 1.38 rad Φ = 0.38 rad Φ 2.9m ϴϴ 0.56m

  5. ϴ = 1.38 rad Φ = 0.38 rad Night Fall @ 18:30 Day Break @ 5:30 0.38*780 π 11:13 – 12:47 94 min 780 min in the day 1.38*780 π 1.38*780 π Φ 12:47 – 18:30 343 min 343 min 5:30 – 11:13 ϴϴ Horizon

  6. So during the time of 11:13 and 12:47 We should be getting the most hits

  7. Computer

  8. Top view

  9. Overall View #1

  10. Overall view #2

  11. Bottom – Bottom veiw

  12. TOP- Bottom view

  13. TOP VIEW

  14. Data

  15. The time we detect the maximum number of muons should be at precisely the peak of the solar day. However is seems to more often be around 1pm.

  16. The amount of muons hitting our detector should increase and decrease in a 24 hour cycle. This does not mean however that at noon there will be a peak in the number of muons produced. Assuming there is a consistent stream of cosmic rays coming in from the sun, then at noon it should peak, although the particles creating the muons in the atmosphere will be much older than the light we see because the particles travel slower. There are other factors in the amount of muons, for example as the distance between the earth and sun increases or decreases.

  17. list of causes of changes in # of cosmic rays solar day (roughly 24 hour cycle what we were looking at) 11 years Schwabe cycle(increase/decrease in sunspots) 22 years Hale cycle(suns poles full revolution of suns poles)

More Related