相较于单涡旋光束，涡旋阵列光束能够扩充信息的传输容量，研究其传输特性对其光通信应用具有重要意义。本文选取阶数为n的螺旋因斯-高斯(HIG_n,n)模式，采用海上大气折射率变换的功率谱，模拟海面大气湍流。基于相位屏法研究了一维阵列涡旋光束在海面大气湍流中光强、相位、闪烁因子和质心漂移的变化情况。结果表明：（1）HIG_n,n模式的闪烁因子和质心漂移标准差随湍流强度以及大气湍流内尺度的增加而增加；（2）n为奇数的HIG_n,n模式的闪烁因子随着阶数的增大而减小，且高于n为偶数的HIG_n,n模式；（3）阶数n>1的HIG_n,n模式比LG_0,1模式具有更好的稳定性；（4）阶数越高，HIG_n,n模式的质心漂移标准差越小。其次，选取线性阵列涡旋光束（LAVBs）进行对比，研究得出虽然LAVBs比HIG光束具有更好的传输性能，但由于HIG光束具有独特的结构，故可适用于不同的应用场景。最后，分析了椭圆参量和椭圆环数对HIG模式传输的影响，结果表明适当地增大椭圆参量或椭圆环数有助于提高HIG模式的抗湍流能力。本文研究结果对涡旋光束的海上应用具有指导意义。

Multimode photonic quantum memory could enhance the information processing speed in a quantum repeater-based quantum network. A large obstacle that impedes the storage of the spatial multimode in a hot atomic ensemble is atomic diffusion, which severely disturbs the structure of the retrieved light field. In this paper, we demonstrate that the elegant Ince-Gaussian (eIG) mode possesses the ability to resist such diffusion. Our experimental results show that the overall structure of the eIG modes under different parameters maintains well after microseconds of storage. In contrast, the standard IG modes under the same circumstance are disrupted and become unrecognizable. Our findings could promote the construction of quantum networks based on room-temperature atoms.