blobs Lagrange point active region fibrils Faraday cup frozen in sun filaments any Fe emission line butterfly diagram flare Waves heliosheath magnetohydrodynamics (MHD) burst red/blue shift (solar) wind emission spectroscopy chromosphere Alfvén waves CME (coronal mass ejection) transition region active region prominence Ed DeLuca UVCS Filter dynamo photosphere shock plages heliosphere jet ejecta raster scan Radiative halo intensity coronal heating EIS emissivity loop XRT arcade corona Maxwellian distribution emission measure twist sunspot energy partition flux rope flux tube Alfvén speed flux magnetic reconnection network initiation SDO Dynamo solar cycle LASCO instability electron density abundance Wind (instrument) CHIANTI filter kink Hinode effective area Flare STEREO quiet sun magnetic field heliopause AIA SDO blobs Lagrange point active region fibrils Faraday cup frozen in sun filaments any Fe emission line butterfly diagram flare Waves heliosheath magnetohydrodynamics (MHD) burst red/blue shift (solar) wind emission spectroscopy chromosphere Alfvén waves CME (coronal mass ejection) transition region active region prominence Ed DeLuca UVCS Filter dynamo photosphere shock plages heliosphere jet ejecta raster scan Radiative halo intensity coronal heating EIS emissivity loop XRT arcade corona Maxwellian distribution emission measure twist sunspot energy partition flux rope flux tube Alfvén speed flux magnetic reconnection network initiation SDO Dynamo solar cycle LASCO instability electron density abundance Wind (instrument) CHIANTI filter kink Hinode effective area Flare STEREO quiet sun magnetic field heliopause AIA SDO
(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.
blobs
Lagrange point
active region
fibrils
Faraday cup
frozen in
sun
filaments
any Fe emission line
butterfly diagram
flare
Waves
heliosheath
magnetohydrodynamics (MHD)
burst
red/blue shift
(solar) wind
emission
spectroscopy
chromosphere
Alfvén waves
CME (coronal mass ejection)
transition region
active region
prominence
Ed DeLuca
UVCS
Filter
dynamo
photosphere
shock
plages
heliosphere
jet
ejecta
raster scan
Radiative
halo
intensity
coronal heating
EIS
emissivity
loop
XRT
arcade
corona
Maxwellian distribution
emission measure
twist
sunspot
energy partition
flux rope
flux tube
Alfvén speed
flux
magnetic reconnection
network
initiation
SDO
Dynamo
solar cycle
LASCO
instability
electron density
abundance
Wind (instrument)
CHIANTI
filter
kink
Hinode
effective area
Flare
STEREO
quiet sun
magnetic field
heliopause
AIA
SDO