We obtained near-infrared images and spectra of the Jovian aurorae using the CRSP (Cryogenic Spectrometer) on the KPNO 2.1-m telescope on January 22, 1992 (UT). The slit of the CRSP was aligned with (63^{\circ}) north and south latitudes in order to study the spatial structure of the auroral emission between 2 and (4 \mu \mathrm{m}). The spatial resolution was about 3 arcsec with spectral resolving powers of about 1000 and 700 for 2 and (4 \mu \mathrm{m}), respectively. We obtained spatially resolved emission intensities of (1) (\mathrm{H}{3}^{+})fundamental band lines between 3 and (4 \mu \mathrm{m}) and (2) the (\mathrm{H}{2}) quadrupole lines of (Q_{1}(1), Q_{1}(3)), and (S_{1}(1)), and several (H_{3}^{+})lines between 2 and (2.5 \mu \mathrm{m}) in the northern auroral region. The northern bright spot as seen in the 2- (\mu \mathrm{m} \mathrm{H}{2}) and (\mathrm{H}{3}^{+})emission lines is at nearly the same position as the northern bright spot due to the (\mathrm{H}{3}^{+})fundamental band lines. We derived spatially resolved rotational temperatures from the (\mathrm{H}{3}^{+})lines in the north polar region and found that temperatures on the bright spot are no greater than those in other auroral regions. This suggests an enhanced abundance of (\mathrm{H}{3}^{+})on the bright spot relative to other parts of the auroral zone. We found the southern (\mathrm{H}{3}^{+})line intensities to be much lower than those in the northern auroral zone, suggesting a lower level of auroral activity near the south pole at the time of the observations. The continuum near the known (\mathrm{H}_{3}^{+})lines in the 3.17 - to (3.57-\mu \mathrm{m}) region shows a significant brightening around the northern bright spot position, implying that the continuum contains many weak uniden-