STEREO transition region AIA Wind (instrument) magnetic reconnection corona effective area UVCS Maxwellian distribution solar cycle LASCO fibrils butterfly diagram ejecta heliosheath arcade network Faraday cup frozen in emission any Fe emission line flux emission measure intensity Hinode prominence emissivity Alfvén waves active region photosphere flare jet sun shock Waves twist heliosphere instability kink initiation CME (coronal mass ejection) Radiative heliopause flux tube energy partition raster scan quiet sun filter flux rope chromosphere magnetic field XRT spectroscopy burst dynamo Flare Alfvén speed plages magnetohydrodynamics (MHD) CHIANTI coronal heating halo Lagrange point blobs SDO EIS active region red/blue shift Ed DeLuca Filter loop SDO (solar) wind electron density sunspot Dynamo filaments abundance STEREO transition region AIA Wind (instrument) magnetic reconnection corona effective area UVCS Maxwellian distribution solar cycle LASCO fibrils butterfly diagram ejecta heliosheath arcade network Faraday cup frozen in emission any Fe emission line flux emission measure intensity Hinode prominence emissivity Alfvén waves active region photosphere flare jet sun shock Waves twist heliosphere instability kink initiation CME (coronal mass ejection) Radiative heliopause flux tube energy partition raster scan quiet sun filter flux rope chromosphere magnetic field XRT spectroscopy burst dynamo Flare Alfvén speed plages magnetohydrodynamics (MHD) CHIANTI coronal heating halo Lagrange point blobs SDO EIS active region red/blue shift Ed DeLuca Filter loop SDO (solar) wind electron density sunspot Dynamo filaments abundance
(Print) Use this randomly generated list as your call list when playing the game. There is no need to say the BINGO column name. Place some kind of mark (like an X, a checkmark, a dot, tally mark, etc) on each cell as you announce it, to keep track. You can also cut out each item, place them in a bag and pull words from the bag.
STEREO
transition region
AIA
Wind (instrument)
magnetic reconnection
corona
effective area
UVCS
Maxwellian distribution
solar cycle
LASCO
fibrils
butterfly diagram
ejecta
heliosheath
arcade
network
Faraday cup
frozen in
emission
any Fe emission line
flux
emission measure
intensity
Hinode
prominence
emissivity
Alfvén waves
active region
photosphere
flare
jet
sun
shock
Waves
twist
heliosphere
instability
kink
initiation
CME (coronal mass ejection)
Radiative
heliopause
flux tube
energy partition
raster scan
quiet sun
filter
flux rope
chromosphere
magnetic field
XRT
spectroscopy
burst
dynamo
Flare
Alfvén speed
plages
magnetohydrodynamics (MHD)
CHIANTI
coronal heating
halo
Lagrange point
blobs
SDO
EIS
active region
red/blue shift
Ed DeLuca
Filter
loop
SDO
(solar) wind
electron density
sunspot
Dynamo
filaments
abundance