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Coordinate Systems: Alt, El, Az, Zenith Angle ElevationorAltitude Zenith Angle.

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Presentation on theme: "Coordinate Systems: Alt, El, Az, Zenith Angle ElevationorAltitude Zenith Angle."— Presentation transcript:

1 Coordinate Systems: Alt, El, Az, Zenith Angle ElevationorAltitude Zenith Angle

2 Coordinate Systems: Alt, El, Az, Zenith Angle Azimuth

3 Celestial Sphere

4 Coordinates on Celestial Sphere

5 One hemisphere… view from inside

6 Map from inside of Cel. Sphere, looking out

7 Map from inside of Celestial Sphere of radio sky

8 Zero of R.A. coordinate system tied to intersection of Ecliptic Plane with Equatorial Plane The Vernal Equinox

9 Moon’s orbit inclined ~5 deg w.r.t. plane of ecliptic:

10 after ~4.65 (=18.6/4) years, ….

11 after ~9.3 years,…

12 after 18.6 years… Moon orbit has regressed full turn…

13 N.P. Vernal Equinox RA=0 observer’s location Local Siderial Time = LST 6 hours 12 hours 18 hours

14 RA Dec

15 N.P. Vernal Equinox observer’s location LST 6 hours 12 hours 18 hours RA HA HA = Hour Angle

16 N.P. Vernal Equinox observer’s location LST 6 hours 12 hours 18 hours RA HA HA = Hour Angle HA = LST - RA LST = HA

17 N.P. Vernal Equinox RA=0 LST 6 hours 12 hours 18 hours Sun Solar Time = hours since midnight

18 N.P. Vernal Equinox RA=0 GST 6 hours 12 hours 18 hours Sun Greenwich Time …. becomes UTC = Coordinated Universal Time Greenwich

19 N.P. Vernal Equinox RA=0 observer’s location Local Siderial Time = LST 6 hours 12 hours 18 hours

20 One hemisphere: future North Poles

21 Zero of R.A. coordinate system tied to intersection of Ecliptic Plane with Equatorial Plane The Vernal Equinox

22 (at equator, 4 minutes of time = 1 degrees) motion of RA=0, Decl=0 (J2000) in past and future Epochs… Current epoch called `epoch of date’

23 Spherical Trigonometry & Spherical triangles sides are portions of great circles

24 PCD is a spherical triangle PAB is NOT a spherical triangle

25 A c

26 Spherical triangles sin A sin B sin C sin a sin b sin c == cos c = cos a cos b + sin a sin b cos C

27

28 Radio Astronomy Overview Radio `source’ Goals of telescope: maximize collection of energy (sensitivity or gain) isolate source emission from other sources… (directional gain… dynamic range) Collecting area

29 LOFAR “elements”

30 thought experiment… 2 wires out (antennas are “reciprocal” devices… can receive or broadcast)

31 Black Body oven at temperature = T thought experiment …

32 Black Body oven at temperature = T thought experiment … R

33 Black Body oven at temperature = T thought experiment … R … wait a while… reach equilibrium… at T warm resistor delivers power P = kT B (B = frequency bandwidth; k = Boltzmann Const)

34 R real definition… warm resistor produces P = kT B = P a = kT a B temp = T Measure Antenna output Power as “T a ” = antenna temperature TaTa

35 Radio `source’ Collecting area  Reception Pattern or Power Pattern

36 Radio `source’ Collecting area If source with brightness temperature T b fills the beam (reception pattern), then T a = T b (!! No dependence on telescope if emission fills beam !!)

37 receiver “temperature” … quantify Receiver internal noise Power as “T r ” = “receiver temperature” TaTa Ampl, etc T r +T a Ampl, etc Real electronics adds noise …treat as ideal, noise-free amp with added power from warm R

38 “ system temperature” … quantify total receiver System noise power as “T sys ” T sys +T a Ampl, etc RMS fluctuations =  T  T = (fac) T sys /(B t int ) 1/2 Fac ~ 1 – 2 B = Bandwidth, Hz t int = integration time, seconds

39 Radio `point source’ Collecting area Power collected = S A eff B/2 S = flux density (watts/sq-m/Hz) [ 1 Jansky = 1 Jy = 10 -26 w/sq-m/Hz ] A eff = effective area (sq-m) B = frequency bandwith (Hz) T a = S A eff /2k


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