Presentation is loading. Please wait.

Presentation is loading. Please wait.

Big Bear Solar Observatory Michelina and Kaiya.

Published byRalph Lawson Modified over 9 years ago

Similar presentations

Presentation on theme: "Big Bear Solar Observatory Michelina and Kaiya."— Presentation transcript:

1 Big Bear Solar Observatory Michelina and Kaiya

2

3 INSTRUMENTS: GONG: Global Oscillation Network Group, a program to conduct a detailed study the solar internal structure and dynamics (partner) NST: New Solar Telescope, it maps out the granulation of the Sun Varies Spectographs, Filter Imagers, Magnetograph

4 Recent Images: Map of Solar Magnatic Field by the GONG+ instrument taken April 23, '14

5 Recent Images: April 23, 2014 Full Disk H Alpha Simple map of the surface Dark marks- matter falling down Light marks- matter filtering up

6 Recent Images: April 23, 2014 Pulnix CCD Camera Solar Weather/Oscillation

7 Live Feed: www.bbso.njit.edu

Download ppt "Big Bear Solar Observatory Michelina and Kaiya."

Similar presentations

Welcome to the University of Michigan – Dearborn Observatory Founded 2007.

Welcome to the University of Michigan – Dearborn Observatory Founded 2007.
The Sun in all its Glory Here is a look at the sun using many different scanning techniques, as well as different Lenses.

The Sun in all its Glory Here is a look at the sun using many different scanning techniques, as well as different Lenses.
Research School of Astronomy & AstrophysicsSlide 1 SkyMapper SkyMapper and the Stromlo Southern Sky Survey Stefan Keller, Brian Schmidt, Paul Francis and.

Research School of Astronomy & AstrophysicsSlide 1 SkyMapper SkyMapper and the Stromlo Southern Sky Survey Stefan Keller, Brian Schmidt, Paul Francis and.
SOLAR FLARES Marina Rodríguez Baras 1. Solar activity Why do we study it? Close study of the internal processes of a star. Preventing the effects on the.

SOLAR FLARES Marina Rodríguez Baras 1. Solar activity Why do we study it? Close study of the internal processes of a star. Preventing the effects on the.
Big Bear Solar Observatory New Solar Telescope in Big Bear Philip R. Goode Big Bear Solar Observatory Center for Solar-Terrestrial Research New Jersey.

Big Bear Solar Observatory New Solar Telescope in Big Bear Philip R. Goode Big Bear Solar Observatory Center for Solar-Terrestrial Research New Jersey.
Infrastructure and facilities available at INAF – Catania Astrophysical Observatory Salvo Scuderi – INAF OACT 1st SPRING Workshop, Nov 26-28, 2103.

Infrastructure and facilities available at INAF – Catania Astrophysical Observatory Salvo Scuderi – INAF OACT 1st SPRING Workshop, Nov 26-28, 2103.
Martin Crow Crayford Manor House Astronomical Society Planetary observing and Imaging.

Martin Crow Crayford Manor House Astronomical Society Planetary observing and Imaging.
Instructor Notes There is one picture of the Sun in all wavelengths except: Gamma ray – there are no images of the full Sun in gamma ray.

Instructor Notes There is one picture of the Sun in all wavelengths except: Gamma ray – there are no images of the full Sun in gamma ray.
1 Lites FPP-SP Initial Reduct SOT #17 Meeting, NAOJ, April. 2006 Solar-B FPP Initial Data Reduction for the FPP Spectro- Polarimeter October, 2004 Bruce.

1 Lites FPP-SP Initial Reduct SOT #17 Meeting, NAOJ, April Solar-B FPP Initial Data Reduction for the FPP Spectro- Polarimeter October, 2004 Bruce.
Physics 681: Solar Physics and Instrumentation – Lecture 7 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.

Physics 681: Solar Physics and Instrumentation – Lecture 7 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.
Big Bear Solar Observatory / NJIT Active Region Monitor (ARM;www.bbso.njit.edu/arm)  A web-based summary of the latest solar activity (every hour update)

Big Bear Solar Observatory / NJIT Active Region Monitor (ARM;  A web-based summary of the latest solar activity (every hour update)
Show 1 -- photosphere & sunspots SUN COURSE - SLIDE SHOW 3 Show 2 -- corona & solar cycle Today: SOHO.

Show 1 -- photosphere & sunspots SUN COURSE - SLIDE SHOW 3 Show 2 -- corona & solar cycle Today: SOHO.
Astronomical images How they are made, what we can learn from them? Modern telescopes all have instruments attached, starting with cameras. Let’s look.

Astronomical images How they are made, what we can learn from them? Modern telescopes all have instruments attached, starting with cameras. Let’s look.
New Technology Leads to Better and More Detailed Photos of the Sun Sara Whitbeck Physics 1 Fall 2002.

New Technology Leads to Better and More Detailed Photos of the Sun Sara Whitbeck Physics 1 Fall 2002.
The Use of a High School Observatory to study the Metallicity Dependence of the Cepheid Period-Luminosity Relation J. Young, S. Scott, S. M. Kanbur (Physics.

The Use of a High School Observatory to study the Metallicity Dependence of the Cepheid Period-Luminosity Relation J. Young, S. Scott, S. M. Kanbur (Physics.
Big Bear Solar Observatory New Solar Telescope in Big Bear Philip R. Goode Big Bear Solar Observatory Center for Solar-Terrestrial Research New Jersey.

Big Bear Solar Observatory New Solar Telescope in Big Bear Philip R. Goode Big Bear Solar Observatory Center for Solar-Terrestrial Research New Jersey.
Solar Instruments for Observing the Sun David Groski Mt Cuba Observatory.

Solar Instruments for Observing the Sun David Groski Mt Cuba Observatory.
HELAS, Nice 27 September 2006 Visible light Imager and Magnetograph T.Appourchaux on behalf of the VIM team IAS.

HELAS, Nice 27 September 2006 Visible light Imager and Magnetograph T.Appourchaux on behalf of the VIM team IAS.
Observing the Sun. Corona: EUV; X-rays Chromosphere: H , UV, EUV Photosphere: near UV, Visible light, infra-red.

Observing the Sun. Corona: EUV; X-rays Chromosphere: H , UV, EUV Photosphere: near UV, Visible light, infra-red.
1 Future solar missions (Based on the summary by R.A. Harrison) S. Kamio 2004.11.15.

1 Future solar missions (Based on the summary by R.A. Harrison) S. Kamio

Similar presentations

Ads by Google