Correction: Tabata, T., et al. Recalibration of over 35 Years of Infrared and Water Vapor Channel Radiances of the JMA Geostationary Satellites. Remote Sens. 2019, 11, 1189

The authors wish to make the following corrections to this paper [1]:

Tables in the appendix B included errors in copying data. These were corrected.

Replace:

Table without name (Old Table)

Brightness temperature to radiance	Radiance to brightness temperature
$R=\frac{a_1}{exp\left(\frac{a_2}{T_e}-1\right)}$	$T_b=b_0+ b_1{T}_e+b_2{T}_e^2$
where	where
$T_e=b_0+ b_1{T}_b+b_2{T}_b^2$	$T_e=\frac{a_2}{ln\left(\frac{a_1}{R}+1\right)}$

with

Table without name (New Table)

Brightness temperature to radiance	Radiance to brightness temperature
$R=\frac{a_1}{exp\left(\frac{a_2}{T_e}\right)-1}$	$T_b=c_0+ c_1{T}_e+c_2{T}_e^2$
where	where
$T_e=b_0+ b_1{T}_b+b_2{T}_b^2$	$T_e=\frac{a_2}{ln\left(\frac{a_1}{R}+1\right)}$

Replace:

Table A5 (Old Table)

Satellite/ Sensor	Channel	Band Correction Coefficient
		a1	a2	b0	b1	b2
				c0	c1	c2
GMS/ VISSR	IR	8255.7322074	1273.3143667	2.275846	0.988431	1.1793766 × 10−5
				−2.299415	1.011715	−1.2013822 × 10−5
GMS–2/ VISSR	IR	9212.3644250	1320.7100318	1.737134	0.991147	9.4856395 × 10−6
				−1.750673	1.008937	−9.6145107 × 10−6
GMS–3/ VISSR	IR	8186.4103806	1269.7404178	2.223245	0.989076	1.0259023 × 10−5
				−2.245486	1.011059	−1.0452385 × 10−5
GMS–4/ VISSR	IR	9317.5135144	1325.7158559	2.209312	0.989011	1.1303155 × 10−5
				−2.231042	1.011122	−1.1501695 × 10−5
GMS–5/ VISSR	IR	9435.9748564	1331.3105240	0.736362	0.996551	3.0920152 × 10−6
				−0.738703	1.003462	−3.1108864 × 10−6
	WV	35,926.6023447	2078.8468183	0.556851	0.998407	7.5627042 × 10−7
				−0.557728	1.001596	−7.5910270 × 10−7
GOES–9/ Imager	IR	9476.1178904	1333.1957641	0.491152	0.997693	2.0906405 × 10−6
				−0.492194	1.002313	−2.0991027 × 10−6
	WV	38,784.3857168	2132.5673014	0.416589	0.998811	6.0331891 × 10−7
				−0.417077	1.001191	−6.0497125 × 10−7
MTSAT–1R/ JAMI	IR	9472.6233105	1333.0318598	0.402764	0.998122	1.6713304 × 10−6
				−0.403462	1.001882	−1.6769060 × 10−6
	WV	38,354.2134967	2124.6536020	0.401309	0.998855	5.7482986 × 10−7
				−0.401762	1.001147	−5.7635116 × 10−7
MTSAT–2/ IMAGER	IR	9717.8743052	1344.4382687	0.512600	0.997626	2.1027280 × 10−6
				−0.513724	1.002381	−2.1116295 × 10−6
	WV	38,726.0971362	2131.4984293	0.521928	0.998541	6.7803280 × 10−7
				−0.522681	1.001462	−6.8037191 × 10−7

with

Table A5 (New Table)

Satellite/ Sensor	Channel	Band Correction Coefficient
		a1	a2	b0	b1	b2
				c0	c1	c2
GMS/ VISSR	IR	8255.3989526	1273.2972334	2.2757022	0.9884318	1.1793267 × 10−5
				−2.2992685	1.0117148	−1.2013300 × 10−5
GMS–2/ VISSR	IR	9214.2439210	1320.7998423	1.7428946	0.9911486	9.4229928 × 10−6
				−1.7565093	1.0089361	−9.5518013 × 10−6
GMS–3/ VISSR	IR	8186.0813819	1269.7234079	2.2231054	0.9890761	1.0258679 × 10−5
				−2.2453430	1.0110581	−1.0452023 × 10−5
GMS–4/ VISSR	IR	9317.0102296	1325.6919859	2.2092520	0.9890098	1.1306309 × 10−5
				−2.2309816	1.0111233	−1.1504885 × 10−5
GMS–5/ VISSR	IR	9436.1509182	1331.3188041	0.7365781	0.9965505	3.0927987 × 10−6
				−0.7389203	1.0034631	−3.1116802 × 10−6
	WV	35,926.6023447	2078.8468183	0.5568513	0.9984068	7.5627042 × 10−7
				−0.5577277	1.0015964	−7.5910270 × 10−7
GOES–9/ Imager	IR	9718.2592835	1344.4560220	0.5130980	0.9976226	2.1068265 × 10−6
				−0.5142247	1.0023838	−2.1157521 × 10−6
	WV	38,729.0279165	2131.5521983	0.5228348	0.9985389	6.7751021 × 10−7
				−0.5235900	1.0014638	−6.7985173 × 10−7
MTSAT–1R/ JAMI	IR	9475.9080697	1333.1859242	0.4912293	0.9976921	2.0915292 × 10−6
				−0.4922710	1.0023139	−2.0999958 × 10−6
	WV	38,784.1056187	2132.5621676	0.4165452	0.9988113	6.0328185 × 10−7
				−0.4170332	1.0011905	−6.0493393 × 10−7
MTSAT–2/ IMAGER	IR	9471.3339906	1332.9715704	0.4036895	0.9981173	1.6749284 × 10−6
				−0.4043903	1.0018867	−1.6805293 × 10−6
	WV	38,352.6325483	2124.6247169	0.4006764	0.9988567	5.7395127 × 10−7
				−0.4011279	1.0011449	−5.7546785 × 10−7

The authors confirm that the corrected errors are not related to the science and methodology presented in the published paper. The authors apologize for any inconvenience caused to the readers by these changes.