<s>
The	O
Sun	O
Watcher	O
using	O
Active	O
Pixel	O
System	O
Detector	O
and	O
Image	O
Processing	O
(	O
SWAP	B-Application
)	O
telescope	O
is	O
a	O
compact	O
extreme-ultraviolet	O
(	O
EUV	O
)	O
imager	O
on	O
board	O
the	O
PROBA-2	O
mission	O
.	O
</s>
<s>
SWAP	B-Application
provides	O
images	O
of	O
the	O
solar	O
corona	O
at	O
a	O
temperature	O
of	O
roughly	O
1	O
million	O
degrees	O
.	O
</s>
<s>
SWAP	B-Application
's	O
coronal	O
mass	O
ejection	O
(	O
CME	O
)	O
watch	O
program	O
has	O
collected	O
images	O
at	O
an	O
improved	O
image	O
cadence	O
(	O
typically	O
1	O
image	O
every	O
few	O
minutes	O
)	O
since	O
the	O
PROBA-2	O
launch	O
in	O
2009	O
.	O
</s>
<s>
SWAP	B-Application
's	O
EUV	O
images	O
of	O
the	O
corona	O
routinely	O
extend	O
beyond	O
2	O
solar	O
radii	O
from	O
the	O
surface	O
of	O
the	O
Sun	O
,	O
much	O
farther	O
than	O
was	O
thought	O
possible	O
before	O
the	O
mission	O
was	O
launched	O
.	O
</s>
<s>
SWAP	B-Application
was	O
built	O
at	O
the	O
Liège	O
Space	O
Center	O
and	O
is	O
operated	O
from	O
the	O
PROBA-2	O
Science	O
Center	O
at	O
the	O
Royal	O
Observatory	O
of	O
Belgium	O
.	O
</s>
<s>
SWAP	B-Application
has	O
been	O
used	O
to	O
study	O
coronal	O
brightspot	O
dynamics	O
.	O
</s>
